BeppoSAX observations of narrow-line Seyfert 1 galaxies

被引:0
作者
Comastri, A
Fiore, F
Guainazzi, M
Matt, G
Stirpe, GM
Zamorani, G
Brandt, WN
Leighly, KM
Piro, L
Molendi, S
Parmar, AN
Siemiginowska, A
Puchnarewicz, EM
机构
[1] Osservatorio Astron Bologna, I-40126 Bologna, Italy
[2] Osserv Astron Roma, I-00040 Monte Porzio Catone, Italy
[3] Nuova Telespazio, Sci Data Ctr, SAX, I-00131 Rome, Italy
[4] Univ Studi Roma Tre, Dipartimento Fis E Amaldi, I-00146 Rome, Italy
[5] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[6] Columbia Univ, Dept Astron, New York, NY 10027 USA
[7] CNR, Ist Astrofis Spaziale, I-00044 Frascati, Italy
[8] CNR, Ist Fis Cosm & Tecnol Relat, I-20133 Milan, Italy
[9] European Space Agcy, Estec, Dept Space Sci, SA,Astrophys Div, NL-2200 AG Noordwijk, Netherlands
[10] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[11] UCL, Mullard Space Sci Lab, Dorking RH5 6NT, Surrey, England
关键词
X-rays : galaxies; galaxies : Seyfert; galaxies : individual : Ton S 180;
D O I
暂无
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on the first spectrum up to 10 keV of the bright narrow-line Seyfert 1 galaxy Ton S 180, obtained with the imaging instruments onboard BeppoSAX. This is the first observed source in a sample of a dozen narrow-line Seyfert 1 galaxies in the BeppoSAX Core Program, We also present and discuss a high quality optical spectrum taken at the 1.5 m telescope at La Silla two months before the BeppoSAX observation. The X-ray spectrum shows a clear hardening above about 2 keV, where a power law with Gamma similar or equal to 2.3 plus an iron line provide a good description of the data. This slope is significantly steeper than the typical one for classical Seyfert 1's and quasars. The best fit line energy is suggestive of highly ionized iron, which would support the idea that the high accretion rate is (one of) the fundamental parameter(s) characterizing the Narrow Line Seyfert 1 phenomenon.
引用
收藏
页码:31 / 37
页数:7
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