Results 11 to 20 of about 1,040 (235)

Stellar formation in Brightest Cluster Galaxies [PDF]

open access: bronzeProceedings of the International Astronomical Union, 2009
AbstractWe study the interplay between stellar population of the Brightest Cluster Galaxies (BCG) and cluster global properties. We use X-ray properties from Chandra, ROSAT and ASCA observations and BCGs spectra from SDSS-DR6. Using STARLIGHT we determined the star formation history of the BCGs and look for relations with the intra-cluster gas ...
Tatiana Zapata Pichinao, G. B. Lima Neto
openalex   +2 more sources

A detection of wobbling brightest cluster galaxies within massive galaxy clusters [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2017
Accepted ...
David Harvey   +3 more
openalex   +5 more sources

Intrinsic Shapes of Brightest Cluster Galaxies

open access: yesThe Astrophysical Journal, 2022
Abstract We discuss the statistical distribution of galaxy shapes and viewing angles under the assumption of triaxiality by deprojecting observed surface brightness profiles of 56 brightest cluster galaxies (BCGs) coming from a recently published large deep-photometry sample.
Stefano de Nicola   +7 more
openaire   +3 more sources

Are Brightest Cluster Galaxies Special?

open access: yesResearch Notes of the AAS, 2023
Abstract A longstanding question when studying Brightest Cluster Galaxies (BCGs) and their evolution is whether their luminosities are statistical extremes of the luminosity distribution of other cluster member galaxies, or whether their luminosities follow a different,“special” distribution.
Savannah Pobre   +3 more
openaire   +1 more source

Brightest Cluster Galaxy Profile Shapes [PDF]

open access: yesThe Astrophysical Journal, 1996
To appear in Ap.J., 16 ...
Graham, Alister   +3 more
openaire   +2 more sources

Evolution of brightest cluster galaxies in X ray clusters [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2002
A recent paper (Burke, Collins & Mann 2000) presents the analysis of the K-band Hubble diagram of 76 brightest cluster galaxies (BCGs) in X-ray clusters and shows that the properties of BCGs depend on the X-ray luminosity (Lx) of their host clusters.
Brough, S.   +4 more
openaire   +4 more sources

An Infrared Survey of Brightest Cluster Galaxies. II. Why are Some Brightest Cluster Galaxies Forming Stars? [PDF]

open access: yesThe Astrophysical Journal, 2008
Quillen et al.(2007) presented an imaging survey with the {\it Spitzer Space Telescope} of 62 brightest cluster galaxies with optical line emission located in the cores of X-ray luminous clusters. They found that at least half of these sources have signs of excess infrared emission. Here we discuss the nature of the IR emission and its implications for
O'Dea, C.P.   +14 more
openaire   +3 more sources

BRIGHTEST CLUSTER GALAXIES AT THE PRESENT EPOCH [PDF]

open access: yesThe Astrophysical Journal, 2014
Accepted for publication in the Astrophysical ...
Tod R. Lauer   +4 more
openaire   +4 more sources

Brightest cluster galaxies: the centre can(not?) hold [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT We explore the persistence of the alignment of brightest cluster galaxies (BCGs) with their local environment. We find that a significant fraction of BCGs do not coincide with the centroid of the X-ray gas distribution and/or show peculiar velocities (they are not at rest with respect to the cluster mean).
Roberto De Propris   +11 more
openaire   +4 more sources

THE LUMINOSITY PROFILES OF BRIGHTEST CLUSTER GALAXIES [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 2011
(Abridged) We have derived detailed R band luminosity profiles and structural parameters for a total of 430 brightest cluster galaxies (BCGs), down to a limiting surface brightness of 24.5 mag/arcsec^2. Light profiles were initially fitted with a Sersic's R^(1/n) model, but we found that 205 (~48) BCGs require a double component model to accurately ...
Donzelli, C. J.   +2 more
openaire   +3 more sources

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