Precision Fe Kα and Fe Kβ Line Spectroscopy of the Seyfert 1.9 Galaxy NGC 2992 with Suzaku-Reference-Cited by-同舟云学术

Precision Fe Kα and Fe Kβ Line Spectroscopy of the Seyfert 1.9 Galaxy NGC 2992 with Suzaku

Published:2007-01-30 Issue:sp1 Volume:59 Page:S283-S299
ISSN:0004-6264
Container-title:Publications of the Astronomical Society of Japan
language:en
Short-container-title:Publ Astron Soc Jpn

Author:

Yaqoob Tahir,Murphy Kendrah D.,Griffiths Richard E.,Haba Yoshito,Inoue Hajime,Itoh Takeshi,Kelley Richard,Kokubun Motohide,Markowitz Alex,Mushotzky Richard,Okajima Takashi,Ptak Andrew,Reeves James,Serlemitsos Peter J.,Takahashi Tadayuki,Terashima Yuichi

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/pasj/article-pdf/59/sp1/S283/17453031/pasj59-S283.pdf

Reference76 articles.

1. Physical Conditions in the Seyfert Galaxy NGC 2992

2. Abundances of the elements: Meteoritic and solar

3. Arnaud K. A. 1996, in ASP Conf. Ser. 101, Astronomical Data Analysis Software and Systems V, ed. Jacoby G. Barnes J. (San Francisco: ASP), 17

4. Photoelectric absorption cross sections with variable abundances

5. X-Ray Fluorescence Yields, Auger, and Coster-Kronig Transition Probabilities

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