Results 71 to 80 of about 24,234 (169)
Formation of the Dark Matter–Deficient S0 Galaxy NGC 4111 under the Tidal Interactions
We present high-sensitivity and large-scale atomic hydrogen (H i ) observations toward lenticular (S0) galaxy NGC 4111 using the Five-hundred-meter Aperture Spherical Radio Telescope.
Mei Ai +10 more
doaj +1 more source
Galaxy groups in the presence of cosmological constant: Increasing the masses of groups
The boundaries of galaxy groups and clusters are defined by the interplay between the Newtonian attractive force and the decoupling from the local expansion of the Universe.
David Benisty +2 more
doaj +1 more source
Encounters between M33 and Present-day M31 Satellites Hint at a Previous Group Accretion
This work investigates whether two known Andromeda (M31) satellites, Pisces (LGS 3) and Andromeda XVI (And XVI), have interacted with M33, M31’s most massive satellite.
Ekta Patel +4 more
doaj +1 more source
The Environment Of Galaxies And Groups Of Galaxies [PDF]
In this thesis, we employ two numerical tools - semi-\ud analytical models and N-body plus hydrodynamical simulations of large scale structure and individual galaxies - to explore the underlying physics governing the formation and evolution of groups of galaxies, and the role of environment in generating polar structures around disk galaxies.\ud \ud ...
openaire
The proximity of the Magellanic Clouds provides the opportunity to study interacting dwarf galaxies near a massive host, and spatial trends in their stellar population properties in particular, with a unique level of detail.
Roger E. Cohen +13 more
doaj +1 more source
HST Proper Motion of Andromeda III. Another Satellite Coorbiting the M31 Satellite Plane
We measure the absolute proper motion of Andromeda III (And III) using Advanced Camera for Surveys/Wide Field Channel and WFPC2 exposures spanning an unprecedented 22 yr time baseline.
Dana I. Casetti-Dinescu +7 more
doaj +1 more source
We present a new measurement of the Hubble constant, H _0 , following the gravitational-wave event GW170817 and Dark Energy Spectroscopic Instrument (DESI) observations.
A. J. Amsellem +58 more
doaj +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
Gas flows between galaxies and the circumgalactic medium (CGM) play a central role in galaxy evolution and can become observable as giant nebulae when illuminated by quasars. We present an ensemble study of nebulae around 30 UV-luminous quasars at z ≈ 0.
Zhuoqi (Will) Liu +22 more
doaj +1 more source

