Results 61 to 70 of about 553,808 (287)

Evolution of the Color-Magnitude Relation in Galaxy Clusters at z ~1 from the ACS Intermediate Redshift Cluster Survey [PDF]

open access: yes, 2008
We apply detailed observations of the Color-Magnitude Relation (CMR) with the ACS/HST to study galaxy evolution in eight clusters at z~1. The early-type red sequence is well defined and elliptical and lenticular galaxies lie on similar CMRs.
Arjen Van der Wel   +98 more
core   +4 more sources

CO in late-type galaxies within the central region of Abell 1367 [PDF]

open access: yes, 2012
We present (CO)-C-12(J = 1-0) and (CO)-C-12(J = 2-1) spectra for 19 bright, late-type galaxies (spirals) in the central region of the galaxy cluster Abell 1367 (z = 0.02) from observations made with the IRAM 30-m telescope.
T. Scott   +5 more
semanticscholar   +1 more source

Two Candidates for Dual AGN in Dwarf-dwarf Galaxy Mergers

open access: yesThe Astrophysical Journal, 2023
Dual active galactic nuclei (DAGN) are important for understanding galaxy-merger-triggered fueling of black holes and the hierarchical growth of structures.
Marko Mićić   +3 more
doaj   +1 more source

On the dust abundance gradients in late-type galaxies - II. Analytical models as evidence for massive interstellar dust growth in SINGS galaxies [PDF]

open access: yes, 2012
We use simple analytical models of the buildup of the dust component and compare these with radial dust distributions derived from observations of SINGS galaxies.
L. Mattsson, A. Andersen
semanticscholar   +1 more source

Halo-model Analysis of the Clustering of Photometrically Selected Galaxies from SDSS

open access: yes, 2009
We measure the angular 2-point correlation functions of galaxies in a volume limited, photometrically selected galaxy sample from the fifth data release of the Sloan Digital Sky Survey.
Abazajian   +42 more
core   +1 more source

Unresolved and diffuse components of X-ray emission and X-ray-to-K-band luminosity ratios in nearby early-type and late-type galaxies [PDF]

open access: yes, 2011
We explore the nature of unresolved X-ray emission in a broad sample of galaxies of all morphological types based on archival Chandra data. After removing bright compact sources, we study LX/LK luminosity ratios of unresolved emission, and compare them ...
Á. Bogdán, M. Gilfanov
semanticscholar   +1 more source

The Evolution of the Cold Gas Fraction in Nearby Clusters’ Ram-pressure-stripped Galaxies

open access: yesThe Astrophysical Journal, 2023
Cluster galaxies are affected by the surrounding environment, which influences, in particular, their gas, stellar content, and morphology. In particular, the ram pressure exerted by the intracluster medium promotes the formation of multiphase tails of ...
Alessia Moretti   +10 more
doaj   +1 more source

The Differences of Star Formation History Between Merging Galaxies and Field Galaxies in the EDR of the SDSS [PDF]

open access: yes, 2007
Based on the catalog of merging galaxies in the Early Data Release (EDR) of the Sloan Digital Sky Survey (SDSS), the differences of star formation history between merging galaxies and field galaxies are studied statistically by means of three ...
Huang, J. S., Luo, Z. J., Shu, C. G.
core   +2 more sources

Dark halo response and the stellar initial mass function in early-type and late-type galaxies [PDF]

open access: yes, 2010
We investigate the origin of the relations between stellar mass and optical circular velocity for early-type galaxies (ETGs) and late-type galaxies (LTGs) – the Faber–Jackson (FJ) and Tully–Fisher (TF) relations.
A. Dutton   +8 more
semanticscholar   +1 more source

Candidate AGNs in Late-Type Galaxies

open access: yes, 2008
We have assembled a sample of 64 late-type spiral galaxies (T types 6.0-9.0, corresponding to Hubble types Scd-Sm) with archival Chandra data. At a signal-to-noise (S/N) threshold of 3, we find 12 objects with X-ray point-source detections in close proximity with the optical or near-infrared position of the nucleus (median offset = 1.6"), suggestive ...
Desroches, Louis-Benoit, Ho, Luis
openaire   +2 more sources

Home - About - Disclaimer - Privacy