Dust-penetrated morphology in the high-redshift universe: Clues from NGC 922

Astronomy and Astrophysics

Volumn 371, Issue 2, 2001, Pages 393-403

  Block, D L ^a   Puerari, I ^b   Takamiya, M ^c   Abraham, R ^d   Stockton, A ^e   Robson, I ^e   Holland, W ^e  

^a UNIVERSITY OF THE WITWATERSRAND   (South Africa)

^b INSTITUTO NACIONAL DE ASTROFÍSICA   (Mexico)

^c GEMINI OBSERVATORY   (United States)

^d UNIVERSITY OF TORONTO   (Canada)

^e UNIVERSITY OF HAWAII   (United States)

Author keywords

Galaxies: individual (NGC 922); Galaxies: kinematics and dynamics; Galaxies: spiral; Galaxies: structure; Methods: numerical

Indexed keywords

EID: 0035325508     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20010081     Document Type: Article

References (35)