Results 61 to 70 of about 5,760 (217)
In this paper we investigate the effect of weak tidal interactions among galaxies in clusters. We obtain the Fokker-Planck coefficients for this process by making use of the impulse approximation. We assume that the outer regions of a galaxy are well described by isotropically distributed stellar orbits with small angular momenta.
openaire +2 more sources
Bar-spheroid interaction in galaxies
The secular evolution of barred galaxies is explored using N-body simulation and linear analysis. In particular, we examine the interaction between bars and spheroidal components of galaxies. According to our calculations, this interaction drives secular transfer of angular momentum from bars to spheroids, primarily through resonant coupling.
Hernquist, Lars, Weinberg, Martin D.
openaire +3 more sources
A Multiwavelength Portrait of the 3C 220.3 Lensed System
The 3C 220.3 system is a rare case of a foreground narrow-line radio galaxy (“galaxy A,” z _A = 0.6850) lensing a background submillimeter galaxy ( z _SMG = 2.221).
Sóley Ó. Hyman +12 more
doaj +1 more source
A Multiwavelength Approach to Constraining the Merger Properties of ACT-CL J0034.4+0225
ACT-CL J0034.4+0225 is a previously unrecognized merging galaxy cluster at z = 0.38588 ± 0.00068. Our primary evidence is provided by a 21 ks Chandra image that shows two surface brightness peaks separated by ∼49″ (259 kpc) surrounded by an extended ...
Peter Doze +12 more
doaj +1 more source
21-cm observations of the interacting galaxies M81 and M82 [PDF]
Geoff Cottrell
openalex +1 more source
Radio Diagnostics Of Galaxy Interactions [PDF]
The Hickson Compact Groups (Hickson 1982) are relatively isolated systems of galaxies with projected separations comparable to the diameters of the galaxies themselves and are an ideal laboratory for the study of the effects of interactions on the various properties of galaxies.
openaire +2 more sources
High-luminosity IRAS galaxies – I. The proportion of IRAS galaxies in interacting systems [PDF]
A. Lawrence +4 more
openalex +1 more source
A Fast Radio Burst in a Compact Galaxy Group at z ∼ 1
FRB 20220610A is a high-redshift fast radio burst (FRB) that has not been observed to repeat. Here, we present rest-frame UV and optical Hubble Space Telescope observations of the field of FRB 20220610A. The imaging reveals seven extended sources, one of
Alexa C. Gordon +16 more
doaj +1 more source

