888 citations
- Instituto de Astrofísica de CanariasES155 papers
- European Southern ObservatoryCL129 papers
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- Space Telescope Science InstituteUS92 papers
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18 papers · 2 filters
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…
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…
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…
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…
Metal-THINGS: On the metallicity and ionization of ULX sources in NGC 925
Maritza A. Lara-López, Igor A. Zinchenko, Leonid S. Pilyugin +13
We present an analysis of the optical properties of three Ultra Luminous X-ray (ULX) sources identified in NGC 925. We use Integral field unit data from the George Mitchel spectrog…
WISDOM project -- VI. Exploring the relation between supermassive black hole mass and galaxy rotation with molecular gas
Mark D. Smith, Martin Bureau, Timothy A. Davis +6
Empirical correlations between the masses of supermassive black holes (SMBHs) and properties of their host galaxies are well-established. Among these is the correlation with the fl…