X-ray and optical-to-infrared follow-up observations of the transient X-ray burster SAX J1810.8-2609

被引：9

作者：

Greiner, J

Castro-Tirado, AJ

Boller, T

Duerbeck, HW

Covino, S

Israel, GL

Linden-Vornle, MJD

Otazu-Porter, X

机构：

[1] Inst Astrophys, D-14482 Potsdam, Germany

[2] INTA, LAEFF, E-28080 Madrid, Spain

[3] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain

[4] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany

[5] Free Univ Brussels, B-1050 Brussels, Belgium

[6] Osservatorio Astron Brera, I-23807 Merate, Italy

[7] Osservatorio Astron Roma, I-00040 Rome, Italy

[8] Astron Observ, Niels Bohr Inst Astron Phys & Geophys, DK-2100 Copenhagen, Denmark

[9] Univ Barcelona, Fac Fis, Dept Astron & Meteorol, E-08028 Barcelona, Spain

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1999年 / 308卷 / 03期

关键词：

accretion; accretion discs; stars : binaries : general; stars : individual : SAX; J1810.8-2609 (= RX J1810.7-2609); infrared : stars; X-rays : stars;

D O I：

10.1046/j.1365-8711.1999.02921.x

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have performed a ROSAT follow-up observation of the X-ray transient SAX J1810.8-2609 on 1998 March 24 and detected a bright X-ray source (named RX J1810.7-2609) which was not detected during the ROSAT all-sky survey in September 1990. Optical-to-infrared follow-up observations of the 10 " radius ROSAT HRI X-ray error box revealed one variable object (R = 19.5 +/- 0.5 on March 13, R > 21.5 on 1998 August 27) which we tentatively propose: as the optical/IR counterpart of RX J1810.7-2609 = SAX J1810.8-2609.

引用

页码：L17 / L21

页数：5

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