284 citations · 2.4k across the 26 of their papers we have counts for
26 papers
Looking ahead to the sky with the Square Kilometre Array: simulating flux densities & resolved radio morphologies of star-forming galaxies
Rosemary T. Coogan, Mark T. Sargent, Anna Cibinel +4
SKA-MID surveys will be the first in the radio domain to achieve clearly sub-arcsecond resolution at high sensitivity over large areas, opening new science applications for galaxy…
Merger induced clump formation in distant infrared luminous starburst galaxies
Antonello Calabrò, Emanuele Daddi, Jérémy Fensch +6
While the formation of stellar clumps in distant galaxies is usually attributed to gravitational violent disk instabilities, we show here that major mergers also represent a compet…
A contribution of star-forming clumps and accreting satellites to the mass assembly of z ~ 2 galaxies
A. Zanella, E. Le Floc'h, C. M. Harrison +14
We investigate the contribution of clumps and satellites to the galaxy mass assembly. We analyzed spatially-resolved Hubble Space Telescope observations (imaging and slitless spect…
The Main Sequence at contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts?
A. Puglisi, E. Daddi, D. Liu +20
ALMA measurements for 93 -selected galaxies at in COSMOS reveal a sizable (\%) population with compact star formation (SF) sizes, lyi…
The MUSE Atlas of Disks (MAD): Resolving Star Formation Rates and Gas Metallicities on < 100pc Scales
Santiago Erroz-Ferrer, C. Marcella Carollo, Mark den Brok +13
We study the physical properties of the ionized gas in local disks using the sample of 38 nearby M Star-Forming Main Sequence (SFMS) galaxies observed so…
Spatial distribution of stellar mass and star formation activity at 0.2<z<1.2 across and along the Main Sequence
Laura Morselli, Paola Popesso, Anna Cibinel +5
High-resolution multi-wavelength photometry is crucial to explore the spatial distribution of star formation in galaxies and understand how these evolve. To this aim, in this paper…