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Artículos de revistas sobre el tema "HD"

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Publicado: 4 de junio de 2021
Última modificación: 10 de marzo de 2023

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1

Dukes, Robert J. y Saul J. Adelman. "Studies of FCAPT uvby Photometry with Period04: The mCP Stars HD 5797, HD 36792, HD 27309, HD 47913, HD 74521, HD 120198, HD 171263, and HD 215441". Publications of the Astronomical Society of the Pacific 130, n.º 986 (15 de marzo de 2018): 044202. http://dx.doi.org/10.1088/1538-3873/aaa952.

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2

Monier, R., M. Gebran y F. Royer. "Four new HgMn stars: HD 18104, HD 30085, HD 32867, and HD 53588". Astronomy & Astrophysics 577 (mayo de 2015): A96. http://dx.doi.org/10.1051/0004-6361/201526106.

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3

Koga, Hisao, Akira Atsuta y Michimasa Aramaki. "HD-PLC". Journal of The Institute of Image Information and Television Engineers 64, n.º 11 (2010): 1580–83. http://dx.doi.org/10.3169/itej.64.1580.

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4

Jones, H. R. A., R. Paul Butler, G. W. Marcy, C. G. Tinney, A. J. Penny, C. McCarthy y B. D. Carter. "Extrasolar planets around HD 196050, HD 216437 and HD 160691". Monthly Notices of the Royal Astronomical Society 337, n.º 4 (21 de diciembre de 2002): 1170–78. http://dx.doi.org/10.1046/j.1365-8711.2002.05787.x.

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5

Fischer, Debra A., Geoffrey W. Marcy, R. Paul Butler, Steven S. Vogt, Bernie Walp y Kevin Apps. "Planetary Companions to HD 136118, HD 50554, and HD 106252". Publications of the Astronomical Society of the Pacific 114, n.º 795 (mayo de 2002): 529–35. http://dx.doi.org/10.1086/341677.

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6

McKellar, A. R. W. "Interference effects in the spectrum of HD: VI: HD–HD, and HD–Kr at room temperature". Canadian Journal of Physics 72, n.º 5-6 (1 de mayo de 1994): 215–24. http://dx.doi.org/10.1139/p94-033.

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The absorption spectrum of the fundamental band of hydrogen deuteride (λ ≈ 2.7 μm) has been studied in pure HD and in mixtures with krypton at moderate densities (1–45 amagat) and room temperature, using a high-resolution Fourier transform infrared spectrometer. The effects that arise from interference between the allowed dipole transition moments of free HD and the dipoles induced during collisions were studied. For HD–HD collisions, the eight transitions from P1(3) to R1(4) were analyzed to determine line positions, intensities, shift and broadening coefficients, and the phase shift parameters that govern the interference effects. Thus the interference phenomenon was studied over a wider range of initial- and final-J values than previously possible, and the systematic dependence of the phase shifts on transition was determined. For HD–Kr collisions, the R1(0) and R1(1) transitions were examined in detail. The spectrum in the region of R1(1) exhibited a realtively broad underlying "plateau" feature that was shown to be due to the presence of impurity CF4 molecules in the Kr sample.
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7

LeBlanc, F., V. Khalack, B. Yameogo, C. Thibeault y I. Gallant. "Project VeSElkA: results of abundance analysis I – HD 71030, HD 95608, HD 116235 and HD 186568". Monthly Notices of the Royal Astronomical Society 453, n.º 4 (10 de septiembre de 2015): 3767–72. http://dx.doi.org/10.1093/mnras/stv1466.

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8

Stateva, I., I. Kh Iliev y J. Budaj. "Abundance analysis of Am binaries and search for tidally driven abundance anomalies - III. HD 116657, HD 138213, HD 155375, HD 159560, HD 196544 and HD 204188". Monthly Notices of the Royal Astronomical Society 420, n.º 2 (13 de diciembre de 2011): 1207–16. http://dx.doi.org/10.1111/j.1365-2966.2011.20108.x.

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9

Iliev, I. K., J. Budaj, M. Fenovcik, I. Stateva y M. T. Richards. "Abundance analysis of Am binaries and search for tidally driven abundance anomalies - II. HD 861, HD 18778, HD 20320, HD 29479, HD 96528 and HD 108651". Monthly Notices of the Royal Astronomical Society 370, n.º 2 (1 de agosto de 2006): 819–27. http://dx.doi.org/10.1111/j.1365-2966.2006.10513.x.

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10

Sadakane, Kozo, Takashi Ohnishi, Michiko Ohkubo y Yoichi Takeda. "Metallicities in Four Planet-Harbouring K-Type Giants: HD 47536, HD 59686, HD 137759, and HD 219449". Publications of the Astronomical Society of Japan 57, n.º 1 (25 de febrero de 2005): 127–33. http://dx.doi.org/10.1093/pasj/57.1.127.

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11

Giguere, Matthew J., Debra A. Fischer, Matthew J. Payne, John M. Brewer, John Asher Johnson, Andrew W. Howard y Howard T. Isaacson. "NEWLY DISCOVERED PLANETS ORBITING HD 5319, HD 11506, HD 75784 AND HD 10442 FROM THE N2K CONSORTIUM". Astrophysical Journal 799, n.º 1 (19 de enero de 2015): 89. http://dx.doi.org/10.1088/0004-637x/799/1/89.

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12

Перминов, А. С. y Э. Д. Кузнецов. "Орбитальная эволюция внесолнечных планетных систем HD 39194, HD 141399 и HD 160691". Астрономический журнал 96, n.º 10 (2019): 795–814. http://dx.doi.org/10.1134/s000462991909007x.

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13

Kiseleva-Eggleton, Ludmila, Eric Bois, Nicolas Rambaux y Rudolf Dvorak. "Global Dynamics and Stability Limits for Planetary Systems around HD 12661, HD 38529, HD 37124, and HD 160691". Astrophysical Journal 578, n.º 2 (20 de octubre de 2002): L145—L148. http://dx.doi.org/10.1086/344706.

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14

Jeong, Gwanghui, Inwoo Han, Myeong-Gu Park, Artie P. Hatzes, Tae-Yang Bang, Shenghong Gu, Jinming Bai y Byeong-Cheol Lee. "A Search for Exoplanets around Northern Circumpolar Stars. IV. Six Planet Candidates to the K Giants, HD 44385, HD 97619, HD 106574, HD 118904, HD 164428, and HD 202432". Astronomical Journal 156, n.º 2 (24 de julio de 2018): 64. http://dx.doi.org/10.3847/1538-3881/aacbc1.

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15

Ment, Kristo, Debra A. Fischer, Gaspar Bakos, Andrew W. Howard y Howard Isaacson. "Radial Velocities from the N2K Project: Six New Cold Gas Giant Planets Orbiting HD 55696, HD 98736, HD 148164, HD 203473, and HD 211810". Astronomical Journal 156, n.º 5 (18 de octubre de 2018): 213. http://dx.doi.org/10.3847/1538-3881/aae1f5.

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16

Karinkuzhi, Drisya, Aruna Goswami, Navin Sridhar, Thomas Masseron y Meenakshi Purandardas. "Chemical analysis of three barium stars: HD 51959, HD 88035, and HD 121447". Monthly Notices of the Royal Astronomical Society 476, n.º 3 (9 de febrero de 2018): 3086–96. http://dx.doi.org/10.1093/mnras/sty320.

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17

Gruberbauer, M., D. Huber, R. Kuschnig, W. W. Weiss, D. B. Guenther, J. M. Matthews, A. F. J. Moffat et al. "MOST observations of the roAp stars HD 9289, HD 99563, and HD 134214". Astronomy & Astrophysics 530 (25 de mayo de 2011): A135. http://dx.doi.org/10.1051/0004-6361/201116736.

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18

Halbedel, Elaine M. "Photometry of three Herbig Be stars - HD 53367, HD 200775, and HD 259431". Publications of the Astronomical Society of the Pacific 101 (noviembre de 1989): 1004. http://dx.doi.org/10.1086/132567.

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19

Sun, Sining y Maria-Eirini Pandelia. "HD-[HD-GYP] Phosphodiesterases: Activities and Evolutionary Diversification within the HD-GYP Family". Biochemistry 59, n.º 25 (4 de junio de 2020): 2340–50. http://dx.doi.org/10.1021/acs.biochem.0c00257.

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20

Lester, Kathryn V., Gail H. Schaefer, Francis C. Fekel, Douglas R. Gies, Todd J. Henry, Wei-Chun Jao, Leonardo A. Paredes et al. "Visual Orbits of Spectroscopic Binaries with the CHARA Array. IV. HD 61859, HD 89822, HD 109510, and HD 191692". Astronomical Journal 164, n.º 6 (1 de noviembre de 2022): 228. http://dx.doi.org/10.3847/1538-3881/ac9385.

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Abstract We present the visual orbits of four spectroscopic binary stars, HD 61859, HD 89822, HD 109510, and HD 191692, using long baseline interferometry with the CHARA Array. We also obtained new radial velocities from echelle spectra using the APO 3.5 m, CTIO 1.5 m, and Fairborn Observatory 2.0 m telescopes. By combining the astrometric and spectroscopic observations, we solve for the full, three-dimensional orbits and determine the stellar masses to 1%–12% uncertainty and distances to 0.4%–6% uncertainty. We then estimate the effective temperature and radius of each component star through Doppler tomography and spectral energy distribution analyses. We found masses of 1.4–3.5 M ⊙, radii of 1.5–4.7 R ⊙, and temperatures of 6400–10,300 K. We then compare the observed stellar parameters to the predictions of the stellar evolution models, but found that only one of our systems fits well with the evolutionary models.
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21

Peterson, R. C., B. Barbuy y M. Spite. "Trans-iron Ge, As, Se, and heavier elements in the dwarf metal-poor stars HD 19445, HD 84937, HD 94028, HD 140283, and HD 160617". Astronomy & Astrophysics 638 (junio de 2020): A64. http://dx.doi.org/10.1051/0004-6361/202037689.

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Context. The spectra of unevolved metal-poor halo stars uniquely reflect the elemental abundances incorporated during the earliest Galactic epoch. Their heavy-element content is well understood as the products of neutron capture on iron-peak elements. However, for the lightest trans-iron elements with atomic number 30 < Z < 52, they show striking abundance patterns that defy model predictions. Understanding their sources may illuminate the diverse halo, thick disk, or extragalactic origins of metal-poor stars. Aims. The primary goal is the derivation of halo dwarf abundances and their uncertainties for six trans-iron elements from UV spectra, plus optical abundances for four additional trans-Fe elements and two well-understood heavier elements. Methods. For five metal-poor dwarfs, we analyzed high-resolution UV spectra from the Hubble Space Telescope Imaging Spectrograph, supplemented by archival optical echelle spectra. Two independent analyses adopted different programs, models, and line lists, clarifying systematic errors. Results. The results from the separate UV analyses are in good agreement. The largest source of discrepancy is the placement of the UV continuum. Once rectified, the separate results agree to 0.2 dex for moderately unblended, moderately strong lines. Similar agreement is found with previous works, except where new data and line selection become important, notably our exclusion of trans-Fe lines blended by newly identifed Fe I lines. Conclusions. Improved line lists lead to low As/Ge ratios that no longer require an early arsenic enhancement. All five stars exhibit a high Mo/Ge abundance ratio, independent of Mo/Fe. The trans-Fe elements show an odd-even effect: an odd-Z element abundance is depressed relative to those of adjacent even-Z elements. Its suggested metallicity dependence is supported by previous studies of Sr-Y-Zr. Some theoretical yields show a metallicity-dependent odd-even effect, but none have predicted a constant Mo/Ge abundance ratio. Our work thus highlights the complexity of predicting the production of light trans-Fe elements in metal-poor stars.
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22

Sinitskii, L. A. y I. M. Romanishin. "HD-Systems". Journal of Automation and Information Sciences 30, n.º 1 (1998): 82–95. http://dx.doi.org/10.1615/jautomatinfscien.v30.i1.70.

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23

Arora, Akhil, Sakshi Sinha, Piyush Kumar y Arnab Bhattacharya. "HD-index". Proceedings of the VLDB Endowment 11, n.º 8 (abril de 2018): 906–19. http://dx.doi.org/10.14778/3204028.3204034.

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24

Fuhry, David, Yang Zhang, Venu Satuluri, Arnab Nandi y Srinivasan Parthasarathy. "PLASMA-HD". Proceedings of the VLDB Endowment 6, n.º 12 (28 de agosto de 2013): 1318–21. http://dx.doi.org/10.14778/2536274.2536305.

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25

Flaxton, Terry. "HD Aesthetics". Convergence: The International Journal of Research into New Media Technologies 17, n.º 2 (mayo de 2011): 113–23. http://dx.doi.org/10.1177/1354856510394884.

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26

VEATCHGOODMAN, L., P. COMO, J. CHA y J. PAULSEN. "Treatment of HD: A Survey of HD Clinicians". Neurotherapeutics 5, n.º 2 (abril de 2008): 374. http://dx.doi.org/10.1016/j.nurt.2007.10.047.

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27

McCarthy, Chris, R. Paul Butler, C. G. Tinney, Hugh R. A. Jones, Geoffrey W. Marcy, Brad Carter, Alan J. Penny y Debra A. Fischer. "Multiple Companions to HD 154857 and HD 160691". Astrophysical Journal 617, n.º 1 (10 de diciembre de 2004): 575–79. http://dx.doi.org/10.1086/425214.

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28

Kremer, H. P. H. "Imaging Huntington's disease (HD) brains - imagine HD trials!" Journal of Neurology, Neurosurgery & Psychiatry 76, n.º 5 (1 de mayo de 2005): 620. http://dx.doi.org/10.1136/jnnp.2004.056267.

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29

Perminov, A. S. y E. D. Kuznetsov. "Orbital Evolution of the Extrasolar Planetary Systems HD 39194, HD 141399, and HD 160691". Astronomy Reports 63, n.º 10 (octubre de 2019): 795–813. http://dx.doi.org/10.1134/s1063772919090075.

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30

Miller, Ricarda E., Toni Rantanen, Kevin A. Ogilvie, Ulrich Groth y Victor Snieckus. "Combined DirectedorthoMetalation−Halogen Dance (HD) Synthetic Strategies. HD−AnionicorthoFries Rearrangement and Double HD Sequences". Organic Letters 12, n.º 10 (21 de mayo de 2010): 2198–201. http://dx.doi.org/10.1021/ol100493v.

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31

Jeong, G., B. C. Lee, I. Han, M. Omiya, H. Izumiura, B. Sato, H. Harakawa, E. Kambe y D. Mkrtichian. "Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996". Astronomy & Astrophysics 610 (febrero de 2018): A3. http://dx.doi.org/10.1051/0004-6361/201629185.

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Aims. The purpose of this paper is to detect and investigate the nature of long-term radial velocity (RV) variations of K-type giants and to confirm planetary companions around the stars. Methods. We have conducted two planet search programs by precise RV measurement using the 1.8 m telescope at Bohyunsan Optical Astronomy Observatory (BOAO) and the 1.88 m telescope at Okayama Astrophysical Observatory (OAO). The BOAO program searches for planets around 55 early K giants. The OAO program is looking for 190 G–K type giants. Results. In this paper, we report the detection of long-period RV variations of three K giant stars, HD 40956, HD 111591, and HD 113996. We investigated the cause of the observed RV variations and conclude the substellar companions are most likely the cause of the RV variations. The orbital analyses yield P = 578.6 ± 3.3 d, m sin i = 2.7 ± 0.6 MJ, a = 1.4 ± 0.1 AU for HD 40956; P = 1056.4 ± 14.3 d, m sin i = 4.4 ± 0.4 MJ, a = 2.5 ± 0.1 AU for HD 111591; P = 610.2 ± 3.8 d, m sin i = 6.3 ± 1.0 MJ, a = 1.6 ± 0.1 AU for HD 113996.
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32

Glagolevskij, Yurij V. y Ewald Gerth. "Modelling of three long-periodic magnetic CP-stars: HD 2453, HD 12288, and HD 200311". Proceedings of the International Astronomical Union 2004, IAUS224 (julio de 2004): 614–18. http://dx.doi.org/10.1017/s1743921305009440.

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33

King, J. R. "Lithium Abundances of the Cool Metal-Poor Dwarfs HD 103095, HD 134439, and HD 134440". Publications of the Astronomical Society of the Pacific 109 (julio de 1997): 776. http://dx.doi.org/10.1086/133943.

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34

Fischer, Debra A., Geoffrey W. Marcy, R. Paul Butler, Steven S. Vogt, Gregory W. Henry, Dimitri Pourbaix, Bernard Walp, Anthony A. Misch y Jason T. Wright. "A Planetary Companion to HD 40979 and Additional Planets Orbiting HD 12661 and HD 38529". Astrophysical Journal 586, n.º 2 (abril de 2003): 1394–408. http://dx.doi.org/10.1086/367889.

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35

Романовская, А. М., Т. А. Рябчикова y Д. В. Шуляк. "Эволюционный статус Ар-звезд HD 110066 и HD 153882". Письма в астрономический журнал: Астрономия и космическая астрофизика 46, n.º 05 (2020): 353–65. http://dx.doi.org/10.31857/s032001082005006x.

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36

Downing, Nancy R., Spencer Lourens, Isabella De Soriano, Jeffrey D. Long y Jane S. Paulsen. "Phenotype Characterization of HD Intermediate Alleles in PREDICT-HD". Journal of Huntington's Disease 5, n.º 4 (15 de diciembre de 2016): 357–68. http://dx.doi.org/10.3233/jhd-160185.

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37

Boyajian, T. S., T. D. Beaulieu, D. R. Gies, E. Grundstrom, W. Huang, M. V. McSwain, R. L. Riddle, D. W. Wingert y M. De Becker. "The Massive Runaway Stars HD 14633 and HD 15137". Astrophysical Journal 621, n.º 2 (10 de marzo de 2005): 978–84. http://dx.doi.org/10.1086/427650.

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38

Helling, Ch, G. Lee, I. Dobbs-Dixon, N. Mayne, D. S. Amundsen, J. Khaimova, A. A. Unger, J. Manners, D. Acreman y C. Smith. "The mineral clouds on HD 209458b and HD 189733b". Monthly Notices of the Royal Astronomical Society 460, n.º 1 (20 de abril de 2016): 855–83. http://dx.doi.org/10.1093/mnras/stw662.

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39

Hall, Douglas S. y Gregory W. Henry. "Two New Spotted Variables-HD 191262 and HD 191011". Astronomical Journal 104 (noviembre de 1992): 1936. http://dx.doi.org/10.1086/116369.

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40

Strasburger, Krzysztof. "Modified adiabatic approximation: Charge asymmetry in HD+ and HD". Journal of Chemical Physics 131, n.º 13 (7 de octubre de 2009): 134103. http://dx.doi.org/10.1063/1.3241280.

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41

Lu, Wen-xian. "Revised spectroscopic orbits of HD 144515 and HD 178428". Chinese Astronomy and Astrophysics 14, n.º 3 (septiembre de 1990): 282–88. http://dx.doi.org/10.1016/0275-1062(90)90053-g.

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42

Glagolevskii, Yu V. "Magnetic field models for HD 116458 and HD 126515". Astronomy Reports 49, n.º 12 (diciembre de 2005): 1001–8. http://dx.doi.org/10.1134/1.2139816.

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43

Pompéia, L. y D. M. Allen. "HD 11397 and HD 14282: two new barium stars?" Astronomy & Astrophysics 488, n.º 2 (23 de julio de 2008): 723–29. http://dx.doi.org/10.1051/0004-6361:200809707.

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44

Griffin, R. F. y Francis C. Fekel. "HD 115781 and HD 116204—two RS CVn binaries". Journal of Astrophysics and Astronomy 9, n.º 4 (diciembre de 1988): 213–24. http://dx.doi.org/10.1007/bf02715066.

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45

Monnier, John D., Tim J. Harries, Alicia Aarnio, Fred C. Adams, Sean Andrews, Nuria Calvet, Catherine Espaillat et al. "Polarized Disk Emission from Herbig Ae/Be Stars Observed Using Gemini Planet Imager: HD 144432, HD 150193, HD 163296, and HD 169142". Astrophysical Journal 838, n.º 1 (20 de marzo de 2017): 20. http://dx.doi.org/10.3847/1538-4357/aa6248.

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46

Fekel, Francis C. y Gregory W. Henry. "Chromospherically Active Stars. XXIV. The Giant, Single-lined Binaries HD 37824, HD 181809, and HD 217188". Astronomical Journal 129, n.º 3 (marzo de 2005): 1669–85. http://dx.doi.org/10.1086/427713.

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47

Pereira, C. B. "Spectroscopic Verification of Barium Dwarf Candidates: The Analysis of HD 8270, HD 13551, and HD 22589". Astronomical Journal 129, n.º 5 (mayo de 2005): 2469–80. http://dx.doi.org/10.1086/428755.

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48

Garufi, A., S. P. Quanz, H. M. Schmid, H. Avenhaus, E. Buenzli y S. Wolf. "Shadows and cavities in protoplanetary disks: HD 163296, HD 141569A, and HD 150193A in polarized light". Astronomy & Astrophysics 568 (agosto de 2014): A40. http://dx.doi.org/10.1051/0004-6361/201424262.

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49

Hill, Michelle L., Teo Močnik, Stephen R. Kane, Gregory W. Henry, Joshua Pepper, Natalie R. Hinkel, Paul A. Dalba et al. "Orbital Refinement and Stellar Properties for the HD 9446, HD 43691, and HD 179079 Planetary Systems". Astronomical Journal 159, n.º 5 (9 de abril de 2020): 197. http://dx.doi.org/10.3847/1538-3881/ab7d33.

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50

Sangani, K. "What, no HD?" Engineering & Technology 4, n.º 14 (8 de agosto de 2009): 32–33. http://dx.doi.org/10.1049/et.2009.1405.

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