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Journal articles on the topic 'Milky Way'

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Published: 4 June 2021
Last updated: 1 August 2024

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1

DANIEL, JENNY. "Milky way." Nature 353, no. 6344 (October 1991): 496. http://dx.doi.org/10.1038/353496b0.

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2

Brady, Bernadette. "Milky Way." Journal of Skyscape Archaeology 8, no. 1 (August 23, 2022): 97–103. http://dx.doi.org/10.1558/jsa.23692.

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3

Silva, Fabio, and Liz Henty. "Milky Way." Journal of Skyscape Archaeology 8, no. 1 (August 23, 2022): 91–92. http://dx.doi.org/10.1558/jsa.23689.

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4

Rossi, Cristina Peri, and Laura Dail. "The Milky Way." Grand Street, no. 62 (1997): 6. http://dx.doi.org/10.2307/25008192.

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5

Gadd, Bernard, and Bill Manhire. "Milky Way Bar." World Literature Today 66, no. 4 (1992): 785. http://dx.doi.org/10.2307/40148819.

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6

Vallée, J. P. "Magnetic Milky Way." EAS Publications Series 56 (2012): 81–86. http://dx.doi.org/10.1051/eas/1256010.

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7

Seidelmann, P. "Milky Way astrometry." Scholarpedia 7, no. 5 (2012): 10578. http://dx.doi.org/10.4249/scholarpedia.10578.

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8

Hsu, Jeremy. "Milky Way Remapped." Scientific American 318, no. 6 (May 15, 2018): 18. http://dx.doi.org/10.1038/scientificamerican0618-18.

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9

López, Alejandro Martín. "“Milky Way Astronomies”." Journal of Skyscape Archaeology 8, no. 1 (August 4, 2022): 131–34. http://dx.doi.org/10.1558/jsa.23699.

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10

B, Nadieh, and Clara M. "Milky Way Census." Scientific American 327, no. 6 (December 2022): 80. http://dx.doi.org/10.1038/scientificamerican1222-80.

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11

D, Nadia. "Milky Way Swarm." Scientific American 30, no. 1s (March 2021): 32. http://dx.doi.org/10.1038/scientificamericanblackholes0221-32.

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12

Friedman, Robert Bryan. "The Milky Way Model." Astronomy Education Review 7, no. 2 (August 2008): 176–80. http://dx.doi.org/10.3847/aer2008037.

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13

Wilkins, Alex. "Rewinding the Milky Way." New Scientist 254, no. 3391 (June 2022): 8. http://dx.doi.org/10.1016/s0262-4079(22)01037-5.

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14

Tirado-Polo, Francisco, Miguel Anzalota, Zeyn Mirza, Christopher Day-Miller, and José Martin-Ortiz. "S3631 The Milky Way." American Journal of Gastroenterology 116, no. 1 (October 2021): S1487. http://dx.doi.org/10.14309/01.ajg.0000788056.69995.c6.

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15

Abbott, Alison. "Spot the Milky Way." Nature 427, no. 6974 (February 2004): 489. http://dx.doi.org/10.1038/427489b.

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16

Chiao, May. "Move over Milky Way." Nature Physics 12, no. 3 (March 2016): 201. http://dx.doi.org/10.1038/nphys3692.

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17

Karim, Munawar, Angelo Tartaglia, and Ashfaque H. Bokhari. "Weighing the Milky Way." Classical and Quantum Gravity 20, no. 13 (June 10, 2003): 2815–25. http://dx.doi.org/10.1088/0264-9381/20/13/326.

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18

Hall, Shannon. "The Milky Way, Transformed." Scientific American 315, no. 6 (November 15, 2016): 14–16. http://dx.doi.org/10.1038/scientificamerican1216-14.

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19

Bhattacharjee, Y. "Unwinding the Milky Way." Science 327, no. 5970 (March 4, 2010): 1194–95. http://dx.doi.org/10.1126/science.327.5970.1194.

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20

Asanok, Kitiyanee, Danielle Fenech, Jane Greaves, Fiona Healy, Melvin Hoare, Kunal Mooley, Raman Prinja, Luiz Rodriguez, Ben Shaw, and Charlie Walker. "Probing the Milky Way." Astronomy & Geophysics 57, no. 3 (May 31, 2016): 3.31–3.35. http://dx.doi.org/10.1093/astrogeo/atw102.

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21

MONCADA, R. O. "The confused Milky Way." Journal of Epidemiology & Community Health 55, no. 6 (June 1, 2001): 369. http://dx.doi.org/10.1136/jech.55.6.369.

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22

Allen, Owen. "Milky Way from Forsayth." Australian Journal of Rural Health 13, no. 4 (August 2005): 259. http://dx.doi.org/10.1111/j.1440-1584.2005.00711.x.

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23

Englmaier, Peter, and Ortwin Gerhard. "Milky Way Gas Dynamics." Celestial Mechanics and Dynamical Astronomy 94, no. 4 (April 2006): 369–79. http://dx.doi.org/10.1007/s10569-006-9003-3.

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24

Kronberg, Philipp P. "Mapping the Milky Way." Nature 370, no. 6486 (July 1994): 179–80. http://dx.doi.org/10.1038/370179a0.

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25

Grebel, Eva K. "The Amazing Milky Way." German Research 36, no. 3 (December 2014): 6–11. http://dx.doi.org/10.1002/germ.201590007.

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26

Means, Hannah H. "Mysterious Milky Way filaments." Physics Today 76, no. 8 (August 1, 2023): 56. http://dx.doi.org/10.1063/pt.3.5298.

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27

Gilliland, Ben. "Mapping the Milky Way." New Scientist 225, no. 3003 (January 2015): 32–35. http://dx.doi.org/10.1016/s0262-4079(15)60076-8.

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28

Tao, Yiting, Michael Lucas, Asanka Perera, Samuel Teague, Eric Warrant, and Javaan Chahl. "A Computer Vision Milky Way Compass." Applied Sciences 13, no. 10 (May 15, 2023): 6062. http://dx.doi.org/10.3390/app13106062.

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The Milky Way is used by nocturnal flying and walking insects for maintaining heading while navigating. In this study, we have explored the feasibility of the method for machine vision systems on autonomous vehicles by measuring the visual features and characteristics of the Milky Way. We also consider the conditions under which the Milky Way is used by insects and the sensory systems that support their detection of the Milky Way. Using a combination of simulated and real Milky Way imagery, we demonstrate that appropriate computer vision methods are capable of reliably and accurately extracting the orientation of the Milky Way under an unobstructed night sky. The technique presented achieves angular accuracy of better then ±2° under moderate light pollution conditions but also demonstrates that higher light pollution levels will adversely effect orientation estimates by systems depending on the Milky Way for navigation.
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29

Boardman, N., G. Zasowski, J. A. Newman, B. Andrews, C. Fielder, M. Bershady, J. Brinkmann, et al. "Are the Milky Way and Andromeda unusual? A comparison with Milky Way and Andromeda analogues." Monthly Notices of the Royal Astronomical Society 498, no. 4 (September 10, 2020): 4943–54. http://dx.doi.org/10.1093/mnras/staa2731.

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ABSTRACT Our Milky Way provides a unique test case for galaxy evolution models because of our privileged position within the Milky Way’s disc. This position also complicates comparisons between the Milky Way and external galaxies, due to our inability to observe the Milky Way from an external point of view. Milky Way analogue galaxies offer us a chance to bridge this divide by providing the external perspective that we otherwise lack. However, overprecise definitions of ‘analogue’ yield little-to-no galaxies, so it is vital to understand which selection criteria produce the most meaningful analogue samples. To address this, we compare the properties of complementary samples of Milky Way analogues selected using different criteria. We find the Milky Way to be within 1σ of its analogues in terms of star formation rate and bulge-to-total ratio in most cases, but we find larger offsets between the Milky Way and its analogues in terms of disc scale length; this suggests that scale length must be included in analogue selections in addition to other criteria if the most accurate analogues are to be selected. We also apply our methodology to the neighbouring Andromeda galaxy. We find analogues selected on the basis of strong morphological features to display much higher star formation rates than Andromeda, and we also find analogues selected on Andromeda’s star formation rate to overpredict Andromeda’s bulge extent. This suggests both structure and star formation rate should be considered when selecting the most stringent Andromeda analogues.
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30

Boardman, N., G. Zasowski, A. Seth, J. Newman, B. Andrews, M. Bershady, J. Bird, et al. "Milky Way analogues in MaNGA: multiparameter homogeneity and comparison to the Milky Way." Monthly Notices of the Royal Astronomical Society 491, no. 3 (November 11, 2019): 3672–701. http://dx.doi.org/10.1093/mnras/stz3126.

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ABSTRACT The Milky Way provides an ideal laboratory to test our understanding of galaxy evolution, owing to our ability to observe our Galaxy over fine scales. However, connecting the Galaxy to the wider galaxy population remains difficult, due to the challenges posed by our internal perspective and to the different observational techniques employed. Here, we present a sample of galaxies identified as Milky Way analogues on the basis of their stellar masses and bulge-to-total ratios, observed as part of the Mapping Nearby Galaxies at Apache Point Observatory survey. We analyse the galaxies in terms of their stellar kinematics and populations as well as their ionized gas contents. We find our sample to contain generally young stellar populations in their outskirts. However, we find a wide range of stellar ages in their central regions, and we detect central active galactic nucleus-like or composite-like activity in roughly half of the sample galaxies, with the other half consisting of galaxies with central star-forming emission or emission consistent with old stars. We measure gradients in gas metallicity and stellar metallicity that are generally flatter in physical units than those measured for the Milky Way; however, we find far better agreement with the Milky Way when scaling gradients by galaxies’ disc scale lengths. From this, we argue much of the discrepancy in metallicity gradients to be due to the relative compactness of the Milky Way, with differences in observing perspective also likely to be a factor.
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31

Netchitailo, Vladimir S. "Center of Milky Way Galaxy." Journal of High Energy Physics, Gravitation and Cosmology 08, no. 03 (2022): 657–76. http://dx.doi.org/10.4236/jhepgc.2022.83048.

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32

Anders, F., C. Chiappini, B. X. Santiago, H. J. Rocha-Pinto, L. Girardi, L. N. da Costa, M. A. G. Maia, et al. "Chemodynamics of the Milky Way." Astronomy & Astrophysics 564 (April 2014): A115. http://dx.doi.org/10.1051/0004-6361/201323038.

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33

Hodges, K. "Mapping the local Milky Way." Science 353, no. 6307 (September 29, 2016): 1509. http://dx.doi.org/10.1126/science.353.6307.1509-a.

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34

Gilmore, Gerry. "Mysteries of the Milky Way." Nature 400, no. 6743 (July 1999): 402–3. http://dx.doi.org/10.1038/22640.

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35

Collins, Nathan. "Escape from the Milky Way." Scientific American 309, no. 6 (November 19, 2013): 20. http://dx.doi.org/10.1038/scientificamerican1213-20.

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36

Grenache, David G. "Arc of the Milky Way." Clinical Chemistry 66, no. 3 (January 30, 2020): 501. http://dx.doi.org/10.1093/clinchem/hvz030.

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37

Giovanelli, R. "HI beyond the Milky Way." EAS Publications Series 15 (2005): 253–70. http://dx.doi.org/10.1051/eas:2005157.

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38

Forbes, Duncan A. "Reverse engineering the Milky Way." Monthly Notices of the Royal Astronomical Society 493, no. 1 (January 29, 2020): 847–54. http://dx.doi.org/10.1093/mnras/staa245.

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ABSTRACT The ages, metallicities, alpha-elements, and integrals of motion of globular clusters (GCs) accreted by the Milky Way from disrupted satellites remain largely unchanged over time. Here we have used these conserved properties in combination to assign 76 GCs to five progenitor satellite galaxies – one of which we dub the Koala dwarf galaxy. We fit a leaky-box chemical enrichment model to the age–metallicity distribution of GCs, deriving the effective yield and the formation epoch of each satellite. Based on scaling relations of GC counts we estimate the original halo mass, stellar mass, and mean metallicity of each satellite. The total stellar mass of the five accreted satellites contributed around 109 M⊙ in stars to the growth of the Milky Way but over 50 per cent of the Milky Way’s GC system. The five satellites formed at very early times and were likely accreted 8–11 Gyr ago, indicating rapid growth for the Milky Way in its early evolution. We suggest that at least three satellites were originally nucleated, with the remnant nucleus now a GC of the Milky Way. 11 GCs are also identified as having formed ex situ but could not be assigned to a single progenitor satellite.
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39

Wenger, Trey V., Dana S. Balser, L. D. Anderson, and T. M. Bania. "Structure in the Milky Way." Proceedings of the International Astronomical Union 13, S334 (July 2017): 381–82. http://dx.doi.org/10.1017/s1743921317007578.

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AbstractThe morphological and chemical structure of the Milky Way today is an important constraint on models of the formation and evolution of the Galaxy. We use H ii regions, the sites of recent massive star formation, to probe both the Galactic spiral structure and the Galactic metallicity structure. H ii regions are the brightest objects in the Galaxy at radio wavelengths and are detected across the entire Galactic disk. We derive the distances to H ii regions using parallax measurements or by deriving kinematic distances. Here we summarize ongoing work to assess the accuracy of kinematic distances and to complete the census of Galactic H ii regions in the Southern sky.
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40

Matteucci, Francesca, Emanuele Spitoni, and Valeria Grisoni. "Highlights in the Milky Way." Proceedings of the International Astronomical Union 13, S334 (July 2017): 298–99. http://dx.doi.org/10.1017/s174392131700789x.

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AbstractWe discuss some important topics concerning the chemical evolution of the Milky Way. In particular, we compare the predictions of theoretical chemical models for our Galaxy with the latest observational data in order to derive constraint on the formation and evolution of the various Galactic components.
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41

Wong, O. I., M. J. Drinkwater, J. B. Jones, M. D. Gregg, and K. C. Freeman. "Mass of the Milky Way." Symposium - International Astronomical Union 220 (2004): 213–14. http://dx.doi.org/10.1017/s0074180900183251.

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We present a new estimate of the mass of the Milky Way based on the escape velocity of a sample of distant stars, about 12 kpc from the Galactic centre and about 5 kpc from the plane of the Galaxy. Our sample is very different from previous escape-velocity studies, being compiled from an all-object spectroscopic survey of a region of sky. the derived mass within 12 kpc of the Galactic centre is (1.3 ±0.3) × 1011M⊙.
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42

Shiga, David. "Milky Way faces midlife crisis." New Scientist 210, no. 2814 (May 2011): 8. http://dx.doi.org/10.1016/s0262-4079(11)61225-6.

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43

Kraan-Korteweg, Renée C., and Ofer Lahav. "Galaxies behind the Milky Way." Scientific American 279, no. 4 (October 1998): 50–57. http://dx.doi.org/10.1038/scientificamerican1098-50.

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44

Freudenreich, Henry. "Deconstructing the Milky Way Galaxy." American Scientist 87, no. 5 (1999): 418. http://dx.doi.org/10.1511/1999.36.832.

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45

Drimmel, Ronald. "Gaia Reveals the Milky Way." American Scientist 106, no. 5 (2018): 298. http://dx.doi.org/10.1511/2018.106.5.298.

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46

Blitz, Leo. "CO in the Milky Way." Symposium - International Astronomical Union 170 (1997): 11–18. http://dx.doi.org/10.1017/s0074180900233998.

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If the CO distribution of the Milky Way is described as a truncated exponential rather than as a molecular ring with some gas at large radii, it becomes easier to understand the evolution of the disk of stars. The star formation rate per unit molecular gas mass is constant as a function of radius, and the H2 depletion time turns out to be only a few percent of the Hubble time. This very short timescale requires that the atomic gas act as a reservoir for the active star forming gas. Because the HI has such a different radial distribution, there must either be infall from outside the Galaxy, an efficient way for the atomic gas in the disk to lose angular momentum, or both, leading to measurable infall or inflow velocities. The truncation radius of CO is probably due to the recently identified stellar bar.
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47

Bambi, C., and A. D. Dolgov. "Antimatter in the Milky Way." Nuclear Physics B 784, no. 1-2 (November 2007): 132–50. http://dx.doi.org/10.1016/j.nuclphysb.2007.06.010.

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48

Battersby, Stephen. "Milky Way mysteries: Antimatter factory." New Scientist 213, no. 2858 (March 2012): 32–33. http://dx.doi.org/10.1016/s0262-4079(12)60837-9.

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49

von Bloh, Werner, Christine Bounama, and Siegfried Franck. "Photosynthesis in the Milky Way." Plant Science 178, no. 6 (June 2010): 485–90. http://dx.doi.org/10.1016/j.plantsci.2010.02.013.

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50

Crane, Leah. "Milky Way devoured another galaxy." New Scientist 243, no. 3240 (July 2019): 12. http://dx.doi.org/10.1016/s0262-4079(19)31356-9.

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