Results 71 to 80 of about 90,146 (207)
Characterizing the Molecular Gas in Infrared Bright Galaxies with CARMA
We present the CO(1–0) maps of 28 infrared-bright galaxies from the Great Observatories All-Sky Luminous Infrared Galaxy Survey (GOALS) taken with the Combined Array for Research in Millimeter Astronomy (CARMA).
Katherine Alatalo +22 more
doaj +1 more source
Statistics of associations among IR galaxies [PDF]
In the course of expanding the search of Kleinmann et. al. (1988) for distant, infrared-luminous objects, the authors noticed (as is often remarked) that a large number of infrared-selected galaxies have close neighbors or show merger characteristics (e ...
Gallimore, Jack F., Keel, William C.
core +1 more source
The large number of star clusters in nearby galaxies permits us to statistically test the predictions of stellar, dust, and gas models. Using Hubble Space Telescope (HST) broadband plus H α imaging combined with JWST near-infrared imaging, we use a total
Kiana F. Henny +18 more
doaj +1 more source
FAINT CO LINE WINGS IN FOUR STAR-FORMING (ULTRA)LUMINOUS INFRARED GALAXIES [PDF]
Adam K. Leroy +5 more
openalex +1 more source
Dwarf Galaxies with Radio-excess Active Galactic Nuclei in the Very Large Array Sky Survey
We present a systematic search for radio active galactic nuclei (AGNs) in dwarf galaxies using recent observations taken by the Very Large Array Sky Survey (VLASS).
John-Michael Eberhard +4 more
doaj +1 more source
Evolution of the Unidentified Infrared Bands in the Nucleus of the Starburst Galaxy NGC 1097 [PDF]
R. Wu, F. Galliano, Takashi Onaka
openalex +1 more source
Spitzer view on the evolution of star-forming galaxies from z=0 to z~3
We use a 24 micron selected sample containing more than 8,000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3.
Almudena Alonso‐Herrero +25 more
core +1 more source
Near ultraviolet–infrared colours of red-sequence galaxies in local clusters [PDF]
Tim Rawle +4 more
openalex +1 more source
Modern surveys present us with billions of faint galaxies for which we only have broadband images in ∼6–8 optical-to-near-infrared (NIR) filters. Galaxy star formation rates (SFRs) are difficult to estimate accurately without spectroscopic diagnostics or
Yu-Heng Lin +9 more
doaj +1 more source
Star-forming galaxies at high redshift show anomalous values of infrared excess, which can be described only by extremizing the existing relations between the shape of their ultraviolet continuum emission and their infrared-to-ultraviolet luminosity ...
Mancini, Mattia +3 more
core +1 more source

