Results 31 to 40 of about 2,094,644 (376)
Triggering Star Formation by Galaxy-Galaxy Interactions [PDF]
We analyzed the effects of having a close companion on the star formation activity of galaxies in the 8K galaxy pair catalog selected from the 2dFGRS. We found that, statistically, galaxies with rp < 25h−1 kpc and ΔV < 100km s−1 have enhanced star formation with respect to isolated galaxies with the same luminosity and redshift distribution.
M. S. Alonso+3 more
openaire +3 more sources
Searching for TeV Dark Matter in Irregular Dwarf Galaxies with HAWC Observatory
We present the results of dark matter (DM) searches in a sample of 31 dwarf irregular (dIrr) galaxies within the field of view of the HAWC Observatory.
R. Alfaro+72 more
doaj +1 more source
What is driving the evolution of the far-infrared radio correlation? [PDF]
Far infrared-radio correlation represents a linear relationship between far-infrared (FIR) and radio emission in star-forming galaxies. Previous observations have confirmed that this correlation is maintained over a large range of redshift and ...
Pavlović Marina S.+1 more
doaj +1 more source
S0 Galaxies: Outer Gas Accretion through Tidal Interaction and Minor Merging
To clarify the sources of outer gas accretion onto disk galaxies, we study the vicinity of four interacting galaxy systems in the Hα emission line by using the scanning Fabry–Perot interferometer of the 6m telescope of the Special Astrophysical ...
Olga Sil’chenko+3 more
doaj +1 more source
Dwarf Galaxy Formation Induced by Galaxy Interactions [PDF]
9 pages (including 1 figure), To appear in ApJ, 543 (Part 1) Nov 1, 2000 (ApJ volume Nr was wrong in the previous version ...
Tadashi Okazaki, Yoshiaki Taniguchi
openaire +4 more sources
ALMA CO Clouds and Young Star Complexes in the Interacting Galaxies IC 2163 and NGC 2207 [PDF]
Atacama Large Millimeter Array (ALMA) observations of CO(1-0) emission in the interacting galaxies IC 2163 and NGC 2207 are used to determine the properties of molecular clouds and their association with star-forming regions observed with the Hubble ...
D. Elmegreen+7 more
semanticscholar +1 more source
Galactic interactions and subsequent mergers are a paramount channel for galaxy evolution. In this work, we use the data from 236 star-forming CALIFA galaxies with integrated molecular gas observations in their central region (approximately within an ...
Yeny Garay-Solis+7 more
doaj +1 more source
Self-interacting dark matter on small and large scales
In the self-interacting dark matter paradigm (hereafter SIDM), dark matter (DM) is assumed to have non-gravitational interactions with itself. SIDM has been constrained by observations of galaxy clusters. More recently, measurements of large DM densities
Camila A. Correa
doaj +1 more source
The Formation and Evolution of Star Clusters in Interacting Galaxies [PDF]
Observations of globular clusters show that they have universal lognormal mass functions with a characteristic peak at , but the origin of this peaked distribution is highly debated.
Moupiya Maji+5 more
semanticscholar +1 more source
HIGH STAR FORMATION RATES IN TURBULENT ATOMIC-DOMINATED GAS IN THE INTERACTING GALAXIES IC 2163 AND NGC 2207 [PDF]
CO observations of the interacting galaxies IC 2163 and NGC 2207 are combined with HI, Hα, and 24 μm observations to study the star formation rate (SFR) surface density as a function of the gas surface density.
B. Elmegreen+6 more
semanticscholar +1 more source