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ENHANCED MASS LOSS RATES IN RED SUPERGIANTS AND THEIR IMPACT ON THE CIRCUMSTELLAR MEDIUM
L. Hernández-Cervantes, B. Pérez-Rendón, A. Santillán, G. García-Segura and C. Rodríguez-Ibarra Revista Mexicana de Astronomía y Astrofísica 55(2) 161 (2019) https://doi.org/10.22201/ia.01851101p.2019.55.02.04
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Evolution of rotation in rapidly rotating early-type stars during the main sequence with 2D models
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Applicability of Broad-Band Photometry for Determining the Properties of Stars and Interstellar Extinction
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S. A. Khokhlov, A. S. Miroshnichenko, S. V. Zharikov, N. Manset, A. A. Arkharov, N. Efimova, S. Klimanov, V M. Larionov, A. V. Kusakin, R. I. Kokumbaeva, Ch. T. Omarov, K. S. Kuratov, A. K. Kuratova, R. J. Rudy, E. A. Laag, K. B. Crawford, T. K. Swift, R. C. Puetter, R. B. Perry, S. D. Chojnowski, A. Agishev, D. B. Caton, R. L. Hawkins, A. B. Smith, D. E. Reichart, et al. The Astrophysical Journal 856(2) 158 (2018) https://doi.org/10.3847/1538-4357/aab49d
Detection of [O iii] at z ∼ 3: A Galaxy Above the Main Sequence, Rapidly Assembling Its Stellar Mass
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Applications of machine-learning algorithms for infrared colour selection of Galactic Wolf–Rayet stars
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Sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars
Investigating the Lyman photon escape in local starburst galaxies with the Cosmic Origins Spectrograph★
Svea Hernandez, Claus Leitherer, Médéric Boquien, et al. Monthly Notices of the Royal Astronomical Society 478(1) 1292 (2018) https://doi.org/10.1093/mnras/sty1067
On the X-ray temperature of hot gas in diffuse nebulae
The E-MOSAICS project: simulating the formation and co-evolution of galaxies and their star cluster populations
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On Cepheid Distance Scale Bias Due to Stellar Companions and Cluster Populations
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A Runaway Yellow Supergiant Star in the Small Magellanic Cloud∗
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S. Hubrig, M. Schöller, S. P. Järvinen, M. Küker, A. F. Kholtygin and P. Steinbrunner Astronomische Nachrichten 339(1) 72 (2018) https://doi.org/10.1002/asna.201713457
NGC 3105: a young open cluster with low metallicity