|Table of Contents|

Luminosity Functions for Member Galaxies in Central Region of A2199(PDF)

《南京师大学报（自然科学版）》[ISSN:1001-4616/CN:32-1239/N]

Issue:
2013年01期
Page:
37-42
Research Field:
物理学
Publishing date:

Info

Title:
Luminosity Functions for Member Galaxies in Central Region of A2199
Author(s):
Yan Pengfei1; Yuan Qirong2
(1.School of Mathematics and Physics,Qingdao University of Science & Technology,Qingdao 266061,China) (2.School of Physics and Technology,Nanjing Normal University,Nanjing 210023,China)
Keywords:
cluster of galaxies; member galaxies; luminosity function
PACS:
P141.2
DOI:
-
Abstract:
The composite luminosity functions(LFs)of 343 member galaxies of one Abell radius in the central region of the nearby rich galaxy cluster A2199 in the g、r and i bands are studied,and they are found not to be completely consistent with previous studies of the cluster LFs,and not significantly different from the LFs of field galaxies.Based on the classifications for the member galaxies,the tight correlations of LF with the color distribution and the local number density of galaxies are confirmed.

References:

[1] Abell G O.The distribution of rich clusters of galaxies[J].Astrophysical Journal Supplement,1958,3:211-288.
[2]Biviano A,Durret F,Gerbal D,et al.On the galaxy luminosity function in the central regions of the Coma cluster[J].Astronomy and Astrophysics,1995,297:610-616.
[3]Durret F,Gerbal D,Lobo C,et al.The rich cluster of galaxies ABCG 85.Ⅳ.Emission line galaxies,luminosity function and dynamical properties[J].Astronomy and Astrophysics,1999,343:760-774.
[4]Hütsi G,Einasto J,Tucker D L,et al.Luminosity function and density field of the Sloan and Las Campanas Redshift Survey[J].Astronomy and Astrophysics,2002,(eprint arXiv:)astro-ph/0212327.
[5]Adami C,Durret F,Mazure A,et al.Spatial variations of the optical galaxy luminosity functions and red sequences in the Coma cluster:clues to its assembly history[J].Astronomy and Astrophysics,2007,462(2):411-427.
[6]Schechter P.An analytic expression for the luminosity function for galaxies[J].Astrophysical Journal,1976,203:297-306.
[7]Edwin H.The luminosity function of nebulae.Ⅰ.The luminosity function of resolved nebulae as indicated by their brightest stars[J].Astrophysical Journal,1936,84:158-179.
[8]Kinman T D,Grasdalen G L,Rieke G H.Optical and infrared observations of the Jet of M87[J].Astrophysical Journal,1974,194:1-20.
[9]Lugger P M.Luminosity functions for nine Abell clusters[J].Astrophysical Journal,1986,303:535-555.
[10]Gaidos E J.The galaxy luminosity function from observations of twenty Abell clusters[J].Astronomical Journal,1997,113:117-129.
[11]Dressler A.A comprehensive study of 12 very rich clusters of galaxies.Ⅰ.Photometric technique and analysis of the luminosity function[J].Astrophysical Journal,1978,223:765-775,777,779-787.
[12]Popesso P,Biviano A,Böhringer H,et al.RASS-SDSS galaxy cluster survey.Ⅳ.A ubiquitous dwarf galaxy population in clusters[J].Astronomy and Astrophysics,2006,445(1):29-42.
[13]Lobo C,Biviano A,Durret F,et al.Environmental effects on the Coma cluster luminosity function[J].Astronomy and Astrophysics,1997,317:385-392.
[14]Durret F,Adami C,Lobo C.Environmental effects on the galaxy luminosity function in the cluster of galaxies Abell 496[J].Astronomy and Astrophysics,2002,393:439-444.
[15]Xiao Quanbao,Shao Zhengyi,Zhou Xu.Luminosity function of the cluster of galaxies Abell 566[J].Chinese Journal of Astronomy and Astrophysics,2007,7(5):620-628.
[16]Sandage A,Binggeli B,Tammann G A.Studies of the virgo cluster-part five-luminosity functions of virgo cluster galaxies[J].Astronomical Journal,1985,90(1556):1 759-1 771.
[17]Rines K,Mahdavi A,Geller M J,et al.X-ray-emitting groups in the infall region of Abell 2199[J].Astrophysical Journal,2001,555(2):558-562.
[18]Rines K,Geller M J,Diaferio A,et al.Mass profile of the infall region of the Abell 2199 supercluster[J].Astronomical Journal,2002,124(3):1 266-1 282.
[19]Montero-Dorta Antonio D,Prada Francisco.The SDSS DR6 luminosity functions of galaxies[J].Monthly Notices of the Royal Astronomical Society,2009,399(3):1 106-1 118.
[20]Milne M L,Pritchet C J,Poole G B,et al.The faint end of the luminosity function in the core of the coma cluster[J].Astronomical Journal,2007,133:177-185.
[21]Andreon S.The history of mass assembly of faint red galaxies in 28 galaxy clusters since z=1.3[J].Monthly Notices of the Royal Astronomical Society,2008,386(2):1 045-1 052.
[22]Rines K,Geller M J.Spectroscopic determination of the luminosity function in the galaxy clusters A2199 and virgo[J].Astronomical Journal,2008,135(5):1 837-1 848.
[23]Sánchez-Janssen R,Iglesias-Páramo J,Mañoz-Tunñn C,et al.The V-band luminosity function of galaxies in A2151[J].Astronomy and Astrophysics,2005,434(2):521-530.
[24]Boué G,Adami C,Durret F,et al.The galaxy luminosity function of the Abell 496 cluster and its spatial variations[J].Astronomy and Astrophysics,2008,479(2):335-346.
[25]Garilli B,Maccagni D,Andreon S.Composite luminosity function of cluster galaxies[J].Astronomy and Astrophysics,1999,342:408-416.
[26]Blanton M R,Hogg D W,Bahcall N A,et al.The galaxy luminosity function and luminosity density at redshift z=0.1[J].Astrophysical Journal,2003,592(2):819-838.
[27]Blanton M R,Lupton R H,Schlegel D J,et al.The properties and luminosity function of extremely low luminosity galaxies[J].Astrophysical Journal,2005,631(1):208-230.
[28]Strateva I,IveziDc’ ,Knapp G R,et al.Color separation of galaxy types in the sloan digital sky survey imaging data[J].Astronomical Journal,2001,122(4):1 861-1 874.
[29]Marinoni C,Monaco P,Giuricin G,et al.The nearby optical galaxy sample:the local galaxy luminosity function[J].Astrophysical Journal,1999,521(1):50-63.
[30]Goto T,Okamura S,McKay T A,et al.Composite luminosity functions based on the sloan digital sky survey "Cut and Enhance" galaxy cluster catalog[J].Publications of the Astronomical Society of Japan,2002,54(4):515-525.
[31]Binggeli B,Sandage A,Tammann G A.The luminosity function of galaxies[J].Annual Review of Astronomy and Astrophysics,1988,26:509-560.
[32]Adami C,Ulmer M P,Durret F,et al.A turn-over in the galaxy luminosity function of the Coma cluster core?[J].Astronomy and Astrophysics,2000,353:930-936.
[33]Rakos K D,Schombert J M,Odell A P,et al.Cluster populations in A115 and A2283[J].Astrophysical Journal,2000,540(2):715-725.
[34]Dressler A,Smail I,Poggianti B M,et al.A spectroscopic catalog of 10 distant rich clusters of galaxies[J].Astrophysical Journal Supplement Series,1999,122(1):51-80.
[35]Cowan N B,IveziDc’ .The environment of galaxies at low redshift[J].Astrophysical Journal,2008,674(1):13-16.
[36]Lopez-Cruz O,Yee H K C,Brown J P,et al.Are luminous cD halos formed by the disruption of dwarf galaxies?[J].Astrophysical Journal,1997,475:97-101.
[37]Dressler A.Galaxy morphology in rich clusters-implications for the formation and evolution of galaxies[J].Astrophysical Journal,1980,236:351-365.
[38]Dressler A,Oemler A J,Couch W J,et al.Evolution since Z=0.5 of the morphology-density relation for clusters of galaxies[J].Astrophysical Journal,1997,490:577-591.

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Last Update: 2013-03-31