[ 論文紹介 2002下半期 ]

岡村
Haiman 2002,  Ap.J., 576, L1
"The Detectability of High-Redshift Lyman=a Emission
Lines Prior to the Reionization of the Universe",

 （参）Hyman and Spaans 1999, "Models for Dusty Ly_a Emitters at High Redshift",
       ApJ, 518, 138.

       Miralda-Escide 1998, "Reionization of the Intergalactic Medium and the
       DampingWing of the Gunn-Peterson Trough",
       ApJ, 501, 15.

       Miralda-Escude and Rees 1998, "Searching for the Earliest Galaxies Using 
       the Gunn-Peterson Trough and the Ly_a Emmission Line",
       ApJ, 497, 21


八木
Davies et al. 2002, Nature 418 602
"Black holes constrain varying constants"

Murphy et al. 2001, MNRAS 327 1208
"Possible evidence for a variable fine-structure constant from QSO
 absorption lines: motivations, analysis and results"
など。

仲田
Gomez et al.2002 
 Galaxy Star-Formation As A Function Of Environment 
 In The Early Data Release Of The Sloan Digital Sky Survey
 astro-ph/0210193 


児玉
astro-ph/0210643 van Dokkum et al.
astro-ph/0207360 Balogh et al.
ApJ, 124, 1905 (2001) Lubin et al.

嶋作
Conselice, 2002, ApJ, 573, L5-L8
  The Formation of Low-Mass Cluster Galaxies and the Universal 
  Initial Galaxy Mass Function 

Conselice et al. 2002, AJ, 123, 2246-2260
  Galaxy Populations and Evolution in Clusters. II. 
  Defining Cluster Populations

近傍銀河団の非常に暗い銀河 (MB = -16 ~ -11 mag) は青いもの
から非常に赤いものまである。そのうち非常に赤いものは
明るい早期型銀河が銀河同士の相互作用で質量を失って
できたと仮定し、その仮定の妥当性を考察する。



大浜
J.A.L. Aguerri et al. 2001, A&A 367, 428
 Growth of galactic bulges by mergers

Andredakis et al. 1995, MNRAS 275, 87
 The shape of the luminosity profiles of bulges of spiral galaxies

諸隈
Comerford et al. 2002
 Constraining The Redshift z~6 Quasar Luminosity Function 
 Using Gravitational Lensing
 Aj 580,63

大内
Moustakas & Somerville 2002,  ApJ,577,1
The Masses , Ancestors,And Descentants Of Extremely Red Objects:
Constraints From Spatial Clustering

田中
Barton et al. 2000 ApJ 530,660
Tidally Triggered Star Formation In Close Pairs Of Galaxies

Barton et al. 2002 astro-ph/0209317
Tidally Triggered Star Formation In Close Pairs Of Galaxies 2:
constraints on burst strengths and ages


仲田
The Evolution Of X-Ray Clusters of Galaxies
(Rosati,Bogani and Norman 2002 ARA&A 40,539R)


八木
"The Tully--Fisher relation of cluster spirals at z = 0.83"
   Bo Milvang-Jensen, Alfonso Aragon-Salamanca,
   George K. T. Hau, Inger Jorgensen, Jens Hjorth
(astro-ph/0211598 accepted by MNRAS)

  参考 
  The Evolution of the Tully-Fisher Relation of Spiral Galaxies
  Zegler et al. 2002 (ApJ 564,L69)


岡村
'Distribution of Galaxy Spectral Types in the Sloan Digital Sky Survey'
Yip et al. (SDSS preprint)
１７万個の銀河のスペクトルの主成分解析

'A Survey of z>5.Quasars in te Sloan Digital Sky Survey II:
Discovery of Three Additional Quasars at z>6'
Fan et al. (SDSS preprint)
z=6.43 (highest-z quasar)をふくむ3個の新発見と、以前の3個
を合わせた6個のz>5.7 quasarsによる、個数密度や光度関数の解析