Published July 20, 2015
| Version v1
Journal article
Investigating the nature of IGR J17454–2919 using X-ray and near-infrared observations
Creators
- 1. Istituto Nazionale di Astrofisica, INAF-IASF, Via Bassini 15, I-20133 Milano (Italy)
- 2. Massachusetts Institute of Technology, Kavli Institute for Astrophysics, Cambridge, MA 02139 (United States)
- 3. AIM—Astrophysique, Instrumentation et Modélisation (UMR-E 9005 CEA/DSM-CNRS-Université Paris Diderot) Irfu/Service d'Astrophysique, Centre de Saclay F-91191 Gif-sur-Yvette Cedex (France)
- 4. Istituto Nazionale di Astrofisica, IASF Palermo, Via U. La Malfa 153, I-90146 Palermo (Italy)
- 5. Max-Planck-Institute for Extraterrestrial Physics, D-85741 Garching (Germany)
- 6. National Space Institute, Technical University of Denmark, Elektrovej 327-328, DK-2800 Kgs Lyngby (Denmark)
- 7. Thüringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenburg (Germany)
Description
IGR J17454−2919 is a hard X-ray transient discovered by INTEGRAL on 2014 September 27. We report on our 20 ks Chandra observation of the source, performed about five weeks after the discovery, as well as on INTEGRAL and Swift long-term monitoring observations.
Availability note (English)
Available from http://dx.doi.org/10.1088/0004-637X/808/1/34Additional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 808
- Journal Issue
- 1
- Journal Page Range
- [9 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 51041677
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ACCRETION DISKS; HARD X RADIATION; MONITORING; STARS; TRANSIENTS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS; X RADIATION