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EMU Detection of a Large and Low Surface Brightness Galactic SNR G288.8–6.3
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A Severe Challenge to the Modified Newtonian Dynamics Phenomenology in Our Galaxy
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J. V. Sales-Silva, S. Daflon, K. Cunha, D. Souto, V. V. Smith, C. Chiappini, J. Donor, P. M. Frinchaboy, D. A. García-Hernández, C. Hayes, S. R. Majewski, T. Masseron, R. P. Schiavon, D. H. Weinberg, R. L. Beaton, J. G. Fernández-Trincado, H. Jönsson, R. R. Lane, D. Minniti, A. Manchado, C. Moni Bidin, C. Nitschelm, J. O’Connell and S. Villanova The Astrophysical Journal 926(2) 154 (2022) https://doi.org/10.3847/1538-4357/ac4254
Constraining density and metallicity of the Milky Way’s hot gas halo from O vii spectra and ram-pressure stripping
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The Chocolate Chip Cookie Model: Dust Geometry of Milky Way–like Disk Galaxies
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Self-consistent interpretations of the multiwavelength gamma-ray spectrum of LHAASO
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Formation rate of LB-1-like systems through dynamical interactions
Ataru Tanikawa, Tomoya Kinugawa, Jun Kumamoto and Michiko S Fujii Publications of the Astronomical Society of Japan 72(3) (2020) https://doi.org/10.1093/pasj/psaa021
warpfield population synthesis: the physics of (extra-)Galactic star formation and feedback-driven cloud structure and emission from sub-to-kpc scales
Eric W Pellegrini, Stefan Reissl, Daniel Rahner, et al. Monthly Notices of the Royal Astronomical Society 498(3) 3193 (2020) https://doi.org/10.1093/mnras/staa2555
From the outside looking in: what can Milky Way analogues tell us about the star formation rate of our own galaxy?
Amelia Fraser-McKelvie, Michael Merrifield and Alfonso Aragón-Salamanca Monthly Notices of the Royal Astronomical Society 489(4) 5030 (2019) https://doi.org/10.1093/mnras/stz2493
Three-dimensional Structure of the Milky Way Dust: Modeling of LAMOST Data
Linlin 林林 Li 李, Shiyin 世银 Shen 沈, Jinliang 金良 Hou 侯, Haibo 海波 Yuan 苑, Maosheng 茂盛 Xiang 向, Bingqiu 丙秋 Chen 陈, Yang 样 Huang 黄 and Xiaowei 晓为 Liu 刘 The Astrophysical Journal 858(2) 75 (2018) https://doi.org/10.3847/1538-4357/aabaef
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Guangtun Ben Zhu, Jorge K. Barrera-Ballesteros, Timothy M. Heckman, et al. Monthly Notices of the Royal Astronomical Society 468(4) 4494 (2017) https://doi.org/10.1093/mnras/stx740
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The dustier early-type galaxies deviate from late-type galaxies’ scaling relations
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NONUNIVERSAL STAR FORMATION EFFICIENCY IN TURBULENT ISM
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Mercedes Mollá, Oscar Cavichia, Marta Gavilán and Brad K. Gibson Monthly Notices of the Royal Astronomical Society 451(4) 3693 (2015) https://doi.org/10.1093/mnras/stv1102
IMPROVED ESTIMATES OF THE MILKY WAY’S STELLAR MASS AND STAR FORMATION RATE FROM HIERARCHICAL BAYESIAN META-ANALYSIS
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Variation in the dust emissivity index across M 33 withHerschelandSpitzer(HerM 33es)
A thin diffuse component of the Galactic ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries
The RMS survey: galactic distribution of massive star formation★
J. S. Urquhart, C. C. Figura, T. J. T. Moore, et al. Monthly Notices of the Royal Astronomical Society 437(2) 1791 (2014) https://doi.org/10.1093/mnras/stt2006
A review of the chemical abundances and kinematics of the Galactic bulge