参考文献/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-Tunñn 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,IveziDc’ ,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,IveziDc’ .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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