The ORFEUS II Echelle spectrum of HD 93521: A reference for interstellar molecular hydrogen

被引:11
作者
Barnstedt, J
Gringel, W
Kappelmann, N
Grewing, M
机构
[1] Univ Tubingen, Inst Astron & Astrophys, Abt Astron, D-72076 Tubingen, Germany
[2] Inst Radio Astron Millimetr, F-38406 St Martin Dheres, France
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 2000年 / 143卷 / 02期
关键词
stars : individual : HD 93521; ISM : lines and bands; ISM : molecules; ultraviolet : ISM; ultraviolet : stars;
D O I
10.1051/aas:2000176
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
During the second flight of the ORFEUS-SPAS mission in November/December 1996, the Echelle spectrometer was used extensively by the: Principal and Guest Investigator teams as one of the two focal plane instruments of the ORFEUS telescope. The spectrum of IID 93521 was obtained during this mission with a total integration time of 1740s. This spectrum shows numerous sharp interstellar absorption lines. We identified 198 lines of molecular hydrogen including at least 7 lines with a high velocity component. Also most of the 67 identified interstellar metal lilies are visible with a high velocity component. We present; plots of the complete ORFEUS II Echelle spectrum together with tables of all identified interstellar absorption lines including all 14 detectable H I lines. In addition several identified stellar lines, partially with narrow absorption components, anti stellar wind lines are given in a separate table.
引用
收藏
页码:193 / 210
页数:18
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