Starbursts Are Preferentially Interacting: Confirmation from the Nearest Galaxies
We complement a recent Letter by Luo et al. by comparing the fraction of starburst galaxies that are interacting with the overall fraction of interacting...
Statistics and properties of H II regions in NGC 6814
We present a new H-alpha image of high quality of the grand-design galaxy NGC 6814, and describe statistical properties of the H II region population. We have...
Status of the Stratospheric Observatory for Infrared Astronomy (SOFIA)
The Stratospheric Observatory for Infrared Astronomy (SOFIA) is now performing scientific observations and the results of the second open observing cycle...
Stellar and Gas Kinematics in the Core and Bar Regions of M100
Two-dimensional maps of the stellar and gas kinematics of the bar and starbursting circumnuclear region in the barred spiral galaxy M100 are presented. In this...
Using HI Nearby Galaxy Survey (THINGS) 21-cm observations of a sample of nearby (nearly face-on) galaxies we explore whether the stellar disk truncation...
Stellar mass-metallicity relation throughout the large-scale structure of the Universe: CAVITY mother sample
Context. Void galaxies are essential for understanding the physical processes that drive galaxy evolution because they are less affected by external factors...
Stellar masses of giant clumps in CANDELS and simulated galaxies using machine learning
A significant fraction of high redshift star-forming disc galaxies are known to host giant clumps, whose nature and role in galaxy evolution are yet to be...
Stellar masses of star-forming galaxies at 0.3 < z < 1.2 in the GOYA survey
Starforming galaxies with compact morphology and high optical luminosity (LBCGs) are very common at redshitfs z = 0.4 - 1.2. Those galaxies are believed to have...