output
19982026
most citedRotating Massive Main-Sequence Stars I: Grids of Evolutionary Models and Isochrones

888 citations

Showing 2020Show all

73 papers · 1 filter

astro-ph.GA2020★ 6 cited

The Carina Nebula and Gum 31 molecular complex III: The distribution of the 1-3 GHz radio continuum across the whole nebula

David Rebolledo, Anne J. Green, Michael G. Burton +2

We report the most detailed GHz radio continuum emission map of the nearest region of massive star formation, the Carina Nebula. As part of a large program with the Australia…

astro-ph.GA2020★ 6 cited

Two types of distribution of the gas velocity dispersion of MaNGA galaxies

L. S. Pilyugin, I. A. Zinchenko, M. A. Lara-Lopez +2

The distribution of the gas velocity dispersion sigma across the images of 1146 MaNGA galaxies is analyzed. We find that there are two types of distribution of the gas velocity dis…

astro-ph.GA2020★ 31 cited

A dearth of young and bright massive stars in the Small Magellanic Cloud

A. Schootemeijer, N. Langer, D. Lennon +7

Massive star evolution at low metallicity is closely connected to many fields in high-redshift astrophysics, but poorly understood. The Small Magellanic Cloud (SMC) is a unique lab…

astro-ph.GA2020★ 20 cited

Galaxy And Mass Assembly (GAMA): the interplay between galaxy mass, SFR and heavy element abundance in paired galaxy sets

L. E. Garduño, M. A. Lara-López, O. López-Cruz +4

We study the star formation rate (SFR), stellar mass () and the gas metallicity (Z) for 4,636 galaxy pairs using the Galaxy And Mass Assembly (GAMA) survey. Our galaxy p…

astro-ph.IM2020★ 20 cited

The Gravitational-wave Optical Transient Observer (GOTO)

Martin J. Dyer, Danny Steeghs, Duncan K. Galloway +12

The Gravitational-wave Optical Transient Observer (GOTO) is a wide-field telescope project focused on detecting optical counterparts to gravitational-wave sources. GOTO uses arrays…

astro-ph.SR2020★ 49 cited

Wind-envelope interaction as the origin of the slow cyclic brightness variations of luminous blue variables

Luca Grassitelli, Norbert Langer, Jonathan Mackey +4

Luminous blue variables (LBVs) are hot, very luminous massive stars displaying large quasi-periodic variations in brightness, radius,and photospheric temperature, on timescales of…