Thematische Bibliographien / RED II / Zeitschriftenartikel
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Zeitschriftenartikel zum Thema „RED II“

Autor: Grafiati
Veröffentlicht am 28. Juni 2021
Zuletzt aktualisiert am 27. April 2022

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1

Tüzün, Yalçın, und Ronni Wolf. „Red face revisited: II“. Clinics in Dermatology 32, Nr. 6 (November 2014): 709–10. http://dx.doi.org/10.1016/j.clindermatol.2014.09.001.

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2

Xie, Mingyi, und Jörg Bungert. „When Pol II sees red“. Blood 138, Nr. 18 (04.11.2021): 1648–49. http://dx.doi.org/10.1182/blood.2021012453.

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3

Moutray, J. B., und J. L. Mansfield. „Registration of ‘Redland II’ Red Clover“. Crop Science 25, Nr. 4 (Juli 1985): 708. http://dx.doi.org/10.2135/cropsci1985.0011183x002500040039x.

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4

Barlow, F. „William II: Rufus, the Red King“. English Historical Review CXXI, Nr. 492 (01.06.2006): 827–29. http://dx.doi.org/10.1093/ehr/cel110.

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5

Niedermair, Fabian, Roman Trattnig, Kurt Mereiter, Martin Schmuck, Stefan Sax, Emil J. W. List und Christian Slugovc. „Red electrophosphorescent platinum(II) quinolinolate complexes“. Monatshefte für Chemie - Chemical Monthly 141, Nr. 8 (30.07.2010): 847–58. http://dx.doi.org/10.1007/s00706-010-0345-x.

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6

Al-Jan Abi, Monther Y., Subhi S. Al-Azawe und Alia Salman. „Alizarine red s complexes of Mn(II), Co(II) AND Ni(II)“. Thermochimica Acta 113 (März 1987): 209–15. http://dx.doi.org/10.1016/0040-6031(87)88325-9.

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7

Sayre, Hannah J., Agustin Millet, Kim R. Dunbar und Claudia Turro. „Photocatalytic H2production by dirhodium(ii,ii) photosensitizers with red light“. Chemical Communications 54, Nr. 60 (2018): 8332–34. http://dx.doi.org/10.1039/c8cc03631d.

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8

Apak, Reşat, Kubilay Güçlü und Mehmet Hulusi Turgut. „Modeling of Copper(II), Cadmium(II), and Lead(II) Adsorption on Red Mud“. Journal of Colloid and Interface Science 203, Nr. 1 (Juli 1998): 122–30. http://dx.doi.org/10.1006/jcis.1998.5457.

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9

Provan, Drew, und David Weatherall. „Red cells II: acquired anaemias and polycythaemia“. Lancet 355, Nr. 9211 (April 2000): 1260–68. http://dx.doi.org/10.1016/s0140-6736(00)02099-7.

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10

Connan, R. „Type II ostertagiosis in farmed red deer“. Veterinary Record 128, Nr. 10 (09.03.1991): 233–35. http://dx.doi.org/10.1136/vr.128.10.233.

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11

Arbatov, Alexei. „Start II, Red Ink, and Boris Yeltsin“. Bulletin of the Atomic Scientists 49, Nr. 3 (April 1993): 16–21. http://dx.doi.org/10.1080/00963402.1993.11456327.

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12

Pellerin, Patrice, Thierry Doco, Stéphane Vida, Pascale Williams, Jean-Marc Brillouet und Malcolm A. O'Neill. „Structural characterization of red wine rhamnogalacturonan II“. Carbohydrate Research 290, Nr. 2 (September 1996): 183–97. http://dx.doi.org/10.1016/0008-6215(96)00139-5.

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13

Immara Nuur Alfianisa. „Diplomasi Ekonomi Indonesia dalam Merespon RED II“. Jurnal Indonesia Sosial Sains 2, Nr. 8 (21.08.2021): 1271–85. http://dx.doi.org/10.36418/jiss.v2i8.384.

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Lahan Kelapa Sawit yang sangat luas menjadikan Indonesia sebagai pengeskpor kelapa sawit terbesar di dunia. Pada tahun 2017 kelapa sawit menyumbang devisa kepada Negara sebesar USD 23 Miliar atau setara sekitar Rp 300 Triliun, ekspor pada tahun 2017 naik 26% dari tahun sebelumnya. Pada tahun 2020 nilai ekspor kelapa sawit mencapai USD 22,97 Miliar atau setara dengan 320,5 Triliun. Pasar ekspor kelapa sawit Indonesia telah menjangkau pada Negara-Negara besar antara lain China, Uni Eropa dan India. Namun, pada tahun 2017 Uni Eropa merilis kebijakan Delegated Act on Low and High ILUC-Risk Biofuel dalam Renewable Energy Directive (RED II) menggolongkan minyak sawit sebagai indirect land use change-risk biofuel (ILUC). Adanya kebijakan tersebut mendorong Indonesia untuk melakukan strategi diplomasi ekonomi dalam merespon kebijakan tersebut. Adapun diplomasi ekonomi yang dilakukan oleh Indonesia antara lain menghadiri pertemuan nasional maupun internasional seperti menghadiri pertemuan dengan Negara penghasil kelapa sawit, dan Joint Mission di Eropa. Mengupayakan lewat WTO, mengupayakan minyak sawit Indonesia bersertifikat berkelanjutan, mengadakan perjanjian dagang dengan Swiss dan kerjasama produksi kelapa sawit dengan Belanda.
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14

Genet, Jean-Philippe. „John Gillingham, William II: The Red King“. Cahiers de civilisation médiévale, Nr. 239 (01.07.2017): 298–300. http://dx.doi.org/10.4000/ccm.5889.

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15

Gonzalez-Perez, V., C. M. Baugh, C. G. Lacey und J. W. Kim. „Massive, red galaxies in a hierarchical universe - II. Clustering of Extremely Red Objects“. Monthly Notices of the Royal Astronomical Society 417, Nr. 1 (08.08.2011): 517–31. http://dx.doi.org/10.1111/j.1365-2966.2011.19294.x.

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16

Thaler, David S., Elizabeth Sampson, Imran Siddiqi, Susan M. Rosenberg, Lynn C. Thomason, Franklin W. Stahl und Mary M. Stahl. „Recombination of bacteriophage λ in recD mutants of Escherichia coli“. Genome 31, Nr. 1 (01.01.1989): 53–67. http://dx.doi.org/10.1139/g89-013.

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RecBCD enzyme is centrally important in homologous recombination in Escherichia coli and is the source of ExoV activity. Null alleles of either the recB or the recC genes, which encode the B and C subunits, respectively, manifest no recombination and none of the nuclease functions characteristic of the holoenzyme. Loss of the D subunit, by a recD mutation, likewise results in loss of ExoV activity. However, mutants lacking the D subunit are competent for homologous recombination. We report that the distribution of exchanges along the chromosome of Red−Gam−phage λ is strikingly altered by recD null mutations in the host. When λ DNA replication is blocked, recombination in recD mutant strains is high near λ's right end. In contrast, recombination in isogenic recD+ strains is approximately uniform along λ unless the λ chromosome contains a χ sequence. Recombination in recD mutant strains is focused toward the site of action of a type II restriction enzyme acting in vivo on λ. The distribution of exchanges in isogenic recD+ strains is scarcely altered by the restriction enzyme (unless the phage contains an otherwise silent χ). The distribution of exchanges in recD mutants is strongly affected by λ DNA replication. The distribution of exchanges on λ growing in rec+ cells is not influenced by DNA replication. The exchange distribution along λ in recD mutant cells is independent of χ in a variety of conditions. Recombination in rec+ cells is χ influenced. Recombination in recD mutants depends on recC function, occurs in strains deleted for rac prophage, and is independent of recJ, which is known to be required for λ recombination via the RecF pathway. We entertain two models for recombination in recD mutants: (i) recombination in recD mutants may proceed via double-chain break–repair, as it does in λ's Red pathway and E. coli's RecE pathway; (ii) the RecBC enzyme, missing its D subunit, is equivalent to the wild-type, RecBCD, enzyme after that enzyme has been activated by a χ sequence.Key words: χ sequence, RecBCD pathway, Red pathway, RecBC‡ pathway.
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17

Praveen, R. S., und K. Vijayaraghavan. „Optimization of Cu(II), Ni(II), Cd(II) and Pb(II) biosorption by red marine algaKappaphycus alvarezii“. Desalination and Water Treatment 55, Nr. 7 (18.06.2014): 1816–24. http://dx.doi.org/10.1080/19443994.2014.927334.

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18

Liu, Yan, Pei Qin Peng, Xiao Long Zhu und Xian Qing Ding. „Effect of Paper Mill Sludge on Adsorption and Desorption of Cd(II) and Pb(II) in Paddy Soils“. Advanced Materials Research 955-959 (Juni 2014): 2539–45. http://dx.doi.org/10.4028/www.scientific.net/amr.955-959.2539.

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There are high organic matter and cation exchange capacity (CEC) in paper mill sludge, which can be used efficiently to amend soil properties and promote the growth of crops. The batch method was used to investigate effects of paper sludge on adsorption and desorption of Cd (II) and Pb (II) in two types paddy soil (red soil, purple soil), through adding paper sludge to red soil and purple soil. The results showed that isothermal sorption process of Cd (II) and Pb (II) by soils and paper sludge could be well described by Langmuir equation and Freundlich equation, and all coefficients (r) were higher than 0.9. The purple soil had a higher sorption capacity of Cd (II) and Pb (II) than red soil. The sorption capacities of Cd (II) and Pb (II) in soils increased after added paper sludge, and they reached adsorption equilibrium as the percentages of paper sludge were 10%, 1% in red soil and purple soil, respectively. The desorption capacities of Cd (II) and Pb (II) in soils decreased after added paper sludge, and they reached minimum as the percentages of paper sludge were 5%, 2% in red soil and purple soil, respectively. It was better to immobilize Cd (II) and Pb (II) after added paper sludge, thus paper mill sludge can relieve the migration of heavy metals in soil-crop systems. It can provide a new way for safe using of heavy metal contaminated soil and resource utilization of paper sludge.
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19

Yipmantin, Andrea, Holger J. Maldonado, Martha Ly, Jean Marie Taulemesse und Eric Guibal. „Pb(II) and Cd(II) biosorption on Chondracanthus chamissoi (a red alga)“. Journal of Hazardous Materials 185, Nr. 2-3 (Januar 2011): 922–29. http://dx.doi.org/10.1016/j.jhazmat.2010.09.108.

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20

Huang, Jie, Jiaonan Sun, Yiying Wu und Claudia Turro. „Dirhodium(II,II)/NiO Photocathode for Photoelectrocatalytic Hydrogen Evolution with Red Light“. Journal of the American Chemical Society 143, Nr. 3 (11.01.2021): 1610–17. http://dx.doi.org/10.1021/jacs.0c12171.

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21

Waugh, Scott L. „William II: Rufus, the Red King. Emma Mason“. Speculum 82, Nr. 3 (Juli 2007): 732–33. http://dx.doi.org/10.1017/s0038713400010629.

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22

Lynch, Jane M., und Terry L. Barrett. „Collagenolytic (necrobiotic) granulomas: part II - the ‘red’ granulomas“. Journal of Cutaneous Pathology 31, Nr. 6 (07.06.2004): 409–18. http://dx.doi.org/10.1111/j.0303-6987.2004.00208.x.

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23

Shawl, Stephen J., und Donald J. Bord. „Period determinations for Southern Hemisphere red variables. II“. Astronomical Journal 99 (März 1990): 917. http://dx.doi.org/10.1086/115384.

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24

Deda, Massimo La, Mauro Ghedini, Iolinda Aiello, Teresa Pugliese, Francesco Barigelletti und Gianluca Accorsi. „Organometallic emitting dyes: Palladium(II) nile red complexes“. Journal of Organometallic Chemistry 690, Nr. 4 (Februar 2005): 857–61. http://dx.doi.org/10.1016/j.jorganchem.2004.10.028.

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25

PRESTON, J. M., und J. C. CHEN. „Part II-The Use of Infra-red Radiation“. Journal of the Society of Dyers and Colourists 62, Nr. 12 (22.10.2008): 364–68. http://dx.doi.org/10.1111/j.1478-4408.1946.tb02388.x.

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26

Kim, Dohyeong, und Myungshin Im. „What makes red quasars red?“ Astronomy & Astrophysics 610 (Februar 2018): A31. http://dx.doi.org/10.1051/0004-6361/201731963.

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Red quasars are very red in the optical through near-infrared (NIR) wavelengths, which is possibly due to dust extinction in their host galaxies as expected in a scenario in which red quasars are an intermediate population between merger-driven star-forming galaxies and unobscured type 1 quasars. However, alternative mechanisms also exist to explain their red colors: (i) an intrinsically red continuum; (ii) an unusual high covering factor of the hot dust component, that is, CFHD = LHD∕Lbol, where the LHD is the luminosity from the hot dust component and the Lbol is the bolometric luminosity; and (iii) a moderate viewing angle. In order to investigate why red quasars are red, we studied optical and NIR spectra of 20 red quasars at z ~ 0.3 and 0.7, where the usage of the NIR spectra allowed us to look into red quasar properties in ways that are little affected by dust extinction. The Paschen to Balmer line ratios were derived for 13 red quasars and the values were found to be ~10 times higher than unobscured type 1 quasars, suggesting a heavy dust extinction with AV > 2.5 mag. Furthermore, the Paschen to Balmer line ratios of red quasars are difficult to explain with plausible physical conditions without adopting the concept of the dust extinction. The CFHD of red quasars are similar to, or marginally higher than, those of unobscured type 1 quasars. The Eddington ratios, computed for 19 out of 20 red quasars, are higher than those of unobscured type 1 quasars (by factors of 3−5), and hence the moderate viewing angle scenario is disfavored. Consequently, these results strongly suggest the dust extinction that is connected to an enhanced nuclear activity as the origin of the red color of red quasars, which is consistent with the merger-driven quasar evolution scenario.
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27

Fotiric, Milica, Mihailo Nikolic, Jasminka Milivojevic und Dragan Nikolic. „Selection of red raspberry genotypes (Rubus idaeus L.)“. Journal of Agricultural Sciences, Belgrade 54, Nr. 1 (2009): 11–18. http://dx.doi.org/10.2298/jas0901011f.

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Pomological properties of seedlings obtained by open pollination of Meeker's yellow clone were investigated. From over a 100 seedlings obtained from this progeny, 16 genotypes with red fruits were selected on the Experimental Station 'Radmilovac' that belongs to the Faculty of Agriculture in Belgrade. Dunnett-test was used for single testing of physical and chemical traits of raspberry genotypes. It was found that majority of selected genotypes were in the rank with the standard cultivar Meeker, so the final selection of raspberry genotypes was based on organoleptic characteristics. From 16 examined genotypes nine were selected (I/3/2P, I/6/2, I/8/2, II/2/2P, II/3/4P, II/5/3P, II/8/2, II/8/2P and II/PP/2) for further investigation.
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Noldin, Jose A., James M. Chandler, Mary L. Ketchersid und Garry N. McCauley. „Red Rice (Oryza sativa) Biology. II. Ecotype Sensitivity to Herbicides“. Weed Technology 13, Nr. 1 (März 1999): 19–24. http://dx.doi.org/10.1017/s0890037x00044845.

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Greenhouse studies were conducted to evaluate sensitivity of red rice ecotypes from Arkansas, Louisiana, Mississippi, and Texas to soil- and foliar-applied herbicides. Ecotype response to herbicides was variable. Molinate at 4.48 kg ai/ha controlled red rice ecotypes 92 to 100% and cultivars ‘Lemont,’ ‘Mars,’ and ‘Maybelle’ 39 to 63%. Red rice control with thiobencarb at 4.48 kg ai/ha was at least 89%. The tank mixture of fenoxaprop at 0.08 kg ai/ha plus fluazifop-P at 0.10 kg ai/ha controlled red rice and rice cultivars more than for either herbicide applied alone. Red rice and rice cultivar control with paraquat at 0.70 kg ai/ha was 83 to 100%. Blackhulled red rice TX 4 was less sensitive to paraquat and glufosinate than other ecotypes and cultivars. Glufosinate at 1.12 kg ai/ha was required to provide at least 94% control of ecotype TX 4.
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29

Schwertmann, Udo, Josef Friedl, Helge Stanjek, Enver Murad und Christian Bender Koch. „Iron oxides and smectites in sediments from the Atlantis II Deep, Red Sea“. European Journal of Mineralogy 10, Nr. 5 (05.10.1998): 953–68. http://dx.doi.org/10.1127/ejm/10/5/0953.

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30

Carpenter, K. G. „Fluorescence in the Outer Atmospheres of Red Giant Stars“. International Astronomical Union Colloquium 106 (1989): 372. http://dx.doi.org/10.1017/s0252921100063302.

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The outer atmosphere of a cool red giant star is an ideal locale for the operation of line fluorescence processes. Low plasma densities imply low rates of collisional de-excitation and thus allow radiative decay of levels populated by selective radiative pumping. There are many strong sources of line radiation (i.e. possible pumps) and numerous possible upward transitions from highly populated low-lying levels of abundant elements such as Fe II, thus providing many chance coincidences between potential pumps and lines to be pumped. These conditions ensure that many of the chromospheric emission features observed in the UV spectrum of such a star are affected by fluorescence. Many of the observed emission features originate from energy levels populated solely by radiative fluorescent excitation, including strong lines of S I, O I, CO, Ni II, Si I, Fe I and Fe II, as well as weaker lines from Cr II and Co II. Important pumps active in these atmospheres include hydrogen Lyman alpha, and individual lines of 0 I, C I, Si II, Fe II, and Mg II. In the case of Fe II, there are many additional features arising from upper levels whose populations, although primarily maintained by collisions, are also significantly affected by radiative fluorescent excitation. In fact, there may be virtually no level in Fe II not affected to one degree or another by direct decays or cascades down from levels populated by fluorescence, driven either by Lyman alpha or, in some cases, by lines of Fe II itself (“self-fluorescence“).
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31

Darwish, Yahia Hassan. „The Egyptian Red Crescent Society is 75 years old (II)“. International Review of the Red Cross 27, Nr. 261 (Dezember 1987): 655–58. http://dx.doi.org/10.1017/s0020860400061301.

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Taking part in community-service activities is a natural way for young people to satisfy their aspirations and enables them to shoulder their responsibilities as future citizens.This is why the Egyptian Red Crescent has always endeavoured to make use of young people's abilities, help them to become part of society, show them how they can accomplish useful work for the community and, in so doing, support the International Red Cross and Red Crescent Movement.
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32

Shigeyama, T., K. Iwamoto, I. Hachisu, K. Nomoto und H. Saio. „Instabilities and Mixing in Type II-P and II-b Supernovae“. International Astronomical Union Colloquium 145 (1996): 129–35. http://dx.doi.org/10.1017/s0252921100007995.

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We calculate a nonlinear growth of the Rayleigh-Taylor instability in the exploding red supergiant stars with a two-dimensional hydrodynamical code, and examine how the extent of mixing depends on the progenitor's core mass and the envelope mass. The results are compared with the observations of type II-P supernovae and the recent type Il-b supernova 1993J.
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33

Whitaker, Jennifer Seymour, und Dennis L. Bark. „The Red Orchestra. Vol II: The Case of Africa“. Foreign Affairs 68, Nr. 4 (1989): 218. http://dx.doi.org/10.2307/20044189.

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Rizzo, Stanislao, Laura Cinelli und Alfonso Savastano. „Red-Free Photograph of Argus II in Retinitis Pigmentosa“. Ophthalmology Retina 1, Nr. 4 (Juli 2017): 303. http://dx.doi.org/10.1016/j.oret.2017.01.015.

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35

Bowen, David V., und Doron Chelouche. „THE Mg II CROSS-SECTION OF LUMINOUS RED GALAXIES“. Astrophysical Journal 727, Nr. 1 (30.12.2010): 47. http://dx.doi.org/10.1088/0004-637x/727/1/47.

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36

Burgasser, Adam J., J. Davy Kirkpatrick, James Liebert und Adam Burrows. „The Spectra of T Dwarfs. II. Red Optical Data“. Astrophysical Journal 594, Nr. 1 (September 2003): 510–24. http://dx.doi.org/10.1086/376756.

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37

Stiller, J. W., J. L. Riley und B. D. Hall. „THE EVOLUTION OF RNA POLYMERASE II IN RED ALGAE“. Journal of Phycology 36, s3 (Dezember 2000): 64. http://dx.doi.org/10.1046/j.1529-8817.1999.00001-191.x.

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38

Kent Sprague, Rosamond. „Aristotle on Red Mirrors (On Dreams II 459b24 - 460a23)“. Phronesis 30, Nr. 3 (1985): 323–25. http://dx.doi.org/10.1163/156852885x00138.

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39

Savage (née Roquet-Covarrubias), Sonia, Zhou Jia-Long und Alfred G. Maddock. „The red form of bis(1,10-phenanthroline)dithiocyanatoiron(II)“. J. Chem. Soc., Dalton Trans., Nr. 5 (1985): 991–96. http://dx.doi.org/10.1039/dt9850000991.

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40

Reid, Neill, I. S. Glass und R. M. Catchpole. „A survey for red varibles in the LMC – II“. Monthly Notices of the Royal Astronomical Society 232, Nr. 1 (Mai 1988): 53–79. http://dx.doi.org/10.1093/mnras/232.1.53.

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41

Wannier, P. G., R. Sahai, B. G. Andersson und H. R. Johnson. „Mass loss from red giant stars. II - Carbon stars“. Astrophysical Journal 358 (Juli 1990): 251. http://dx.doi.org/10.1086/168980.

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42

Bonomo, Raffaele P., Antonio De Flora, Enrico Rizzarelli, Anna M. Santoro, Giovanni Tabbí und Michela Tonetti. „Copper(II) complexes encapsulated in human red blood cells“. Journal of Inorganic Biochemistry 59, Nr. 4 (September 1995): 773–84. http://dx.doi.org/10.1016/0162-0134(94)00063-g.

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43

Liuzzo, Vincenzo, Werner Oberhauser und Andrea Pucci. „Synthesis of new red photoluminescent Zn(II)-salicylaldiminato complex“. Inorganic Chemistry Communications 13, Nr. 5 (Mai 2010): 686–88. http://dx.doi.org/10.1016/j.inoche.2010.03.020.

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Zhang, Jie, Lei Wang, Aiguo Zhong, Guobo Huang, Fengshou Wu, Dan Li, Mingyu Teng, Jiali Wang und Deman Han. „Deep red PhOLED from dimeric salophen Platinum(II) complexes“. Dyes and Pigments 162 (März 2019): 590–98. http://dx.doi.org/10.1016/j.dyepig.2018.10.053.

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Kanof, Philip D., Blaine S. Greenwald, Richard C. Mohs und Kenneth L. Davis. „Red blood cell choline. II: Kinetics in alzheimer's disease“. Biological Psychiatry 20, Nr. 4 (April 1985): 375–83. http://dx.doi.org/10.1016/0006-3223(85)90040-x.

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Alksnis, O., und L. Začs. „The violet opacity in the red peculiar stars (II)“. Astrophysics and Space Science 215, Nr. 1 (Mai 1994): 73–82. http://dx.doi.org/10.1007/bf00627461.

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47

Støkken, Anne Marie. „Molander, Anders og Jens-Christian Smeby (red.): Profesjonsstudier II“. Norsk statsvitenskapelig tidsskrift 30, Nr. 01 (11.04.2014): 71–76. http://dx.doi.org/10.18261/issn1504-2936-2014-01-06.

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48

Setyawati, Harsasi, Handoko Darmokoesoemo, Irmina Kris Murwani, Ahmadi Jaya Permana und Faidur Rochman. „Functionalization of Congo red dye as a light harvester on solar cell“. Open Chemistry 18, Nr. 1 (20.04.2020): 287–94. http://dx.doi.org/10.1515/chem-2020-0034.

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AbstractThe demands of ecofriendly technologies to produce a reliable supply of renewable energy on a large scale remains a challenge. A solar cell based on DSSC (Dye-Sensitized Solar Cell) technology is environmentally friendly and holds the promise of a high efficiency in converting sunlight into electricity. This manuscript describes the development of a light harvester system as a main part of a DSSC. Congo red dye has been functionalized with metals (Fe, Co, Ni), forming a series of complexes that serve as a novel light harvester on the solar cell. Metal-congo red complexes have been characterized by UV-VIS and FTIR spectroscopy, and elemental analyses. The performance of metal complexes in capturing photons from sunlight has been investigated in a solar cell device. The incorporation of metals to congo red successfully improved of the congo red efficiency as follows: Fe(II)-congo red, Co(II)-congo red and Ni(II)-congo red had efficiencies of 8.17%, 6.13% and 2.65%, respectively. This research also discusses the effect of metal ions on the ability of congo red to capture energy from sunlight.
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Sankar, Muniappan, Chellaiah Arunkumar und Puttaiah Bhyrappa. „Unusual solvent dependent electronic absorption spectral properties of nickel(II) and copper(II) perhaloporphyrins“. Journal of Porphyrins and Phthalocyanines 08, Nr. 12 (Dezember 2004): 1343–55. http://dx.doi.org/10.1142/s1088424604000702.

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Electronic absorption spectra of divalent metal ( Ni (II) and Cu (II)) complexes of 2,3,7,8,12,13,17,18-octa(bromo/chloro)-5,10,15,20-tetraphenylporphyrins (MOXTPP; X = Br , Cl ) were examined in various solvents. M (II) perhaloporphyrins exhibited dramatic shifts in their optical absorption spectral features relative to the corresponding metallotetraphenylporphyrins, MTPPs. Copper(II) perhaloporphyrins show significant red-shifts of the absorption bands in coordinating solvents relative to that observed for nickel(II) perhaloporphyrins. The large red-shift of the electronic absorption bands and the gain in intensity of the longest wavelength band (Q(0,0)), of Cu (II) perhaloporphyrins in certain coordinating solvents is comparable to that found in meso-tetraphenylporphinatozinc(II), ZnTPP. The solvent dependent spectral features of M (II) perhaloporphyrins are attributed to a coordinative interaction of the solvent with the core metal ion induced by the electron deficient porphyrin macrocycle.
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Origlia, Livia, und Ernesto Oliva. „Red supergiants in star-forming galaxies“. Symposium - International Astronomical Union 193 (1999): 613. http://dx.doi.org/10.1017/s007418090020644x.

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We present some results on the burst properties in star forming galaxies, using near infrared stellar features typical of red supergiants and Brackett nebular lines which trace the presence of luminous H II regions.
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