✦ LIBER ✦

Models for the magnitude-distribution of brightest cluster galaxies

✍ Scribed by J. P. Bernstein; Suketu P. Bhavsar

Publisher: John Wiley and Sons
Year: 2001
Tongue: English
Weight: 278 KB
Volume: 322
Category: Article
ISSN: 0035-8711
DOI: 10.1046/j.1365-8711.2001.04124.x

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The stellar content of brightest cluster

The stellar content of brightest cluster galaxies

✍ P. A. James; B. Mobasher 📂 Article 📅 2000 🏛 John Wiley and Sons 🌐 English ⚖ 329 KB

Anisotropy in the Hubble relation for th

Anisotropy in the Hubble relation for the brightest galaxies in clusters

✍ B. N. G. Guthrie 📂 Article 📅 1976 🏛 Springer Netherlands 🌐 English ⚖ 424 KB

Possible selection effects and their con

Possible selection effects and their consequences on the determination of the model of the Universe from the redshift-magnitude relation of the brightest cluster galaxies

✍ A. Vignato; R. Marcucci 📂 Article 📅 1971 🏛 Springer Netherlands 🌐 English ⚖ 774 KB

The surface brightness and colour–magnit

The surface brightness and colour–magnitude relations for Fornax cluster galaxies

✍ A. M. Karick; M. J. Drinkwater; M. D. Gregg 📂 Article 📅 2003 🏛 John Wiley and Sons 🌐 English ⚖ 706 KB

Modelling the evolution of galaxy cluste

Modelling the evolution of galaxy clustering

✍ C. M. Baugh; A. J. Benson; S. Cole; C. S. Frenk; C. G. Lacey 📂 Article 📅 1999 🏛 John Wiley and Sons 🌐 English ⚖ 200 KB

Ultraviolet color-magnitude relation of

Ultraviolet color-magnitude relation of early-type dwarf galaxies in the Virgo cluster

✍ S. Kim; S.-C. Rey; T. Lisker 📂 Article 📅 2009 🏛 John Wiley and Sons 🌐 English ⚖ 76 KB 👁 1 views

## Abstract We present ultraviolet (UV) color‐magnitude relations (CMRs) for dwarf ellipticals (dEs) and dwarf lenticulars (dS0s) in the Virgo cluster. We used the Galaxy Evolution Explorer (GALEX) GR3 photometric data in far‐ultraviolet (FUV) and near‐ultraviolet (NUV) passbands combined with SDSS