Results 71 to 80 of about 5,760 (217)
Interacting galaxies in the NGC 697 group of galaxies [PDF]
AbstractWe studied the morphology of two brightest members of the nearby NGC 697 group of galaxies, and found evidence of satellite accretion onto the primary galaxy NGC 697 of the group as well as outer and inner irregularities of the only early-type galaxy NGC 680 of the group, which are probably shaped by recent dry merging event(s).
openaire +2 more sources
The Complex Multiwavelength Morphology of the Peculiar Compact Galaxy Group IC 2431
We present new Chandra X-ray imaging spectroscopy of the compact galaxy group IC 2431, and compare with archival ultraviolet, optical, infrared, and radio images. IC 2431 is a starburst system containing three tidally distorted disk galaxies.
Beverly J. Smith +5 more
doaj +1 more source
Activity of Interacting Galaxies Mkn 673: A Close-By “E+A” Galaxy [PDF]
W. Kollatschny, K. J. Fricke
openalex +1 more source
Convolutional neural networks have shown their ability to differentiate between self-interacting dark matter (SIDM) and cold dark matter on galaxy cluster scales.
Zhenyang Huang +3 more
doaj +1 more source
H i, FRB, What’s Your z: The First FRB Host Galaxy Redshift from Radio Observations
Identification and follow-up observations of the host galaxies of fast radio bursts (FRBs) not only help us understand the environments in which the FRB progenitors reside, but also provide a unique way of probing the cosmological parameters using the ...
M. Glowacki +12 more
doaj +1 more source
A Near- and Mid-Infrared Study of the Interacting Galaxy Pair UGC 12914/12915: “Taffy” [PDF]
T. H. Jarrett +4 more
openalex +1 more source
A Galactic-scale Magnetized Wind around a Normal Star-forming Galaxy
Galaxy formation theory identifies superwinds as a key regulator of star formation rates, galaxy growth, and chemical enrichment. Thermal and radiation pressure are known to drive galactic-scale winds in dusty starbursting galaxies (e.g., M82), but ...
A. M. Matthews +7 more
doaj +1 more source
Gas accretion from both the circumgalactic medium (CGM)/intergalactic medium (IGM) and interacting companion galaxy can dilute the gas phase metallicity of a galaxy. However, their relative contribution to the chemical evolution of galaxies remains to be
Yibo Cao, Zhizheng Pan
doaj +1 more source
Near‐Infrared Spectroscopy of Arp Interacting Galaxies [PDF]
L. Vanzi +2 more
openalex +1 more source
The molecular gas content throughout the low-z merger sequence
Exploiting IRAM 30 m CO spectroscopy, we find that SDSS post-merger galaxies display gas fractions and depletion times enhanced by 25-50\%, a mildly increased CO excitation, and standard molecular-to-atomic gas ratios, compared to non-interacting ...
Mark T. Sargent +7 more
doaj +1 more source

