No evidence for variability of intervening absorption lines toward GRB 060206: Implications for the Mg II incidence problem

Publications of the Astronomical Society of Japan

Volumn 61, Issue 2, 2009, Pages 387-394

  Aoki, Kentaro ^a   Totani, Tomonori ^b   Hattori, Takashi ^a   Ohta, Kouji ^b   Kawabata, Koji S ^c   Kobayashi, Naoto ^d   Iye, Masanori ^a   Nomoto, Ken'ichi ^d   Kawai, Nobuyuki ^e  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b KYOTO UNIVERSITY   (Japan)

^c HIROSHIMA UNIVERSITY   (Japan)

^d UNIVERSITY OF TOKYO   (Japan)

^e TOKYO INSTITUTE OF TECHNOLOGY   (Japan)

Author keywords

Galaxies: ISM; Gamma rays: bursts

Indexed keywords

GALAXIES; GAMMA RAYS; MAGNESIUM COMPOUNDS; SIGNAL TO NOISE RATIO; STARS;

ABSORPTION LINES; GALAXIES: ISM; GAMMA RAYS BURSTS; HIGH INCIDENCE; LINE OF SIGHT; LINE STRENGTH; LINES-OF-SIGHT; LOW RESOLUTION OPTICAL SPECTRA; SPECTRA'S; SUBARU TELESCOPES;

IRON COMPOUNDS;

EID: 67650701124     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/61.2.387     Document Type: Article

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