The 0.1-200 keV spectrum of the blazar PKS 2005-489 during an active state

被引:22
作者
Tagliaferri, G
Ghisellini, G
Giommi, P
Celotti, A
Chiaberge, M
Chiappetti, L
Glass, IS
Maraschi, L
Tavecchio, F
Treves, A
Wolter, A
机构
[1] Osserv Astron Brera, I-23807 Merate, Italy
[2] ASI, BeppoSAX Sci Data Ctr, I-00131 Rome, Italy
[3] SISSA, ISAS, I-34014 Trieste, Italy
[4] CNR, Ist Fis Cosm G Occhialini, I-20133 Milan, Italy
[5] S African Astron Observ, Observ 7935, ZA-7935 Cape Town, South Africa
[6] Osserv Astron Brera, I-20121 Milan, Italy
[7] Univ Insubria, Ist Fis, I-22100 Como, Italy
关键词
BL lacertae objects : general; X-rays : galaxies; BL lacertae objects : individual : PKS 2005-489;
D O I
10.1051/0004-6361:20010011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The bright BL Lac object PKS 2005-439 was observed by BeppoSAX on November 1-2, 1998 following an active X-ray state detected by RossiXTE. The source, detected between 0.1 and 200 keV, was in a very high st ate with a continuum well fitted by a steepening spectrum due to synchrotron emission only. Our X-ray spectrum is the flattest ever observed for this source. The different X-ray spectral slopes and fluxes as measured by various satellites, are consistent with relatively little changes of the peak frequency of the synchrotron emission always located below; 10(17) Hz. We discuss these results in the framework; of synchrotron self-Compton models. We found that for the BeppoSAX observation, the synchrotron peak frequency is between 10(15) and 2.5 10(16) Hz, depending in the model assumptions.
引用
收藏
页码:38 / 43
页数:6
相关论文
共 38 条
[1]  
Blandford R. D., 1978, Pittsburgh Conf. on BL Lac Objects, P328
[2]   Observations of a correlated gamma-ray and optical flare for BL lacertae [J].
Bloom, SD ;
Bertsch, DL ;
Hartman, RC ;
Sreekumar, P ;
Thompson, DJ ;
Balonek, TJ ;
Beckerman, E ;
Davis, SM ;
Whitman, K ;
Miller, HR ;
Nair, AD ;
Roberts, LC ;
Tosti, G ;
Massaro, E ;
Nesci, R ;
Maesano, M ;
Montagni, F ;
Jang, M ;
Bock, HA ;
Dietrich, M ;
Herter, M ;
Otterbein, K ;
Pfeiffer, M ;
Seitz, T ;
Wagner, S .
ASTROPHYSICAL JOURNAL, 1997, 490 (02) :L145-L148
[3]   The medium-energy concentrator spectrometer on board the BeppoSAX X-ray astronomy satellite [J].
Boella, G ;
Chiappetti, L ;
Conti, G ;
Cusumano, G ;
DelSordo, S ;
LaRosa, G ;
Maccarone, MC ;
Mineo, T ;
Molendi, S ;
Re, S ;
Sacco, B ;
Tripiciano, M .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 122 (02) :327-340
[4]   BeppoSAX, the wide band mission for X-ray astronomy [J].
Boella, G ;
Butler, RC ;
Perola, GC ;
Piro, L ;
Scarsi, L ;
Bleeker, JAM .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 1997, 122 (02) :299-307
[5]   Spectral evolution of PKS 2155-304 observed with BeppoSAX during an active gamma-ray phase [J].
Chiappetti, L ;
Maraschi, L ;
Tavecchio, F ;
Celotti, A ;
Fossati, G ;
Ghisellini, G ;
Giommi, P ;
Pian, E ;
Tagliaferri, G ;
Treves, A ;
Urry, CM ;
Zhang, YH .
ASTROPHYSICAL JOURNAL, 1999, 521 (02) :552-560
[6]   On the soft X-ray spectra of gamma-loud blazars [J].
Comastri, A ;
Fossati, G ;
Ghisellini, G ;
Molendi, S .
ASTROPHYSICAL JOURNAL, 1997, 480 (02) :534-546
[7]   Infrared variability properties of the blazar 3C 279 [J].
Fan, JH .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1999, 308 (04) :1032-1036
[8]  
FIORE F, 1999, COOKBOOK NFI BEPPOSA
[9]   X-ray emission of Markarian 421: New clues from its spectral evolution. II. Spectral analysis and physical constraints [J].
Fossati, G ;
Celotti, A ;
Chiaberge, M ;
Zhang, YH ;
Chiappetti, L ;
Ghisellini, G ;
Maraschi, L ;
Tavecchio, F ;
Pian, E ;
Treves, A .
ASTROPHYSICAL JOURNAL, 2000, 541 (01) :166-179
[10]   X-ray emission of Markarian 421: New clues from its spectral evolution. I. Temporal analysis [J].
Fossati, G ;
Celotti, A ;
Chiaberge, M ;
Zhang, YH ;
Chiappetti, L ;
Ghisellini, G ;
Maraschi, L ;
Tavecchio, F ;
Pian, E ;
Treves, A .
ASTROPHYSICAL JOURNAL, 2000, 541 (01) :153-165