IGR J19140+098, a new INTEGRAL transient

(2) CEA Saclay; 3); (3) ISDC; (4) Laboratoire d'Astrophysique; Clement Cabanac (4); Diana C. Hannikainen (1); Gilles Henri (4); Jerome Rodriguez (2; Juho Schultz (1); Observatoire de Grenoble)

arxiv: astro-ph/0404327 · v1 · submitted 2004-04-16 · 🌌 astro-ph

IGR J19140+098, a new INTEGRAL transient

Juho Schultz (1) , Diana C. Hannikainen (1) , Osmi Vilhu (1) , Jerome Rodriguez (2 , 3) , Clement Cabanac (4) , Gilles Henri (4) , Pierre-Olivier Petrucci (4)

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Panu Muhli (1) ((1) Observatory University of Helsinki (2) CEA Saclay (3) ISDC (4) Laboratoire d'Astrophysique Observatoire de Grenoble)

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classification 🌌 astro-ph

keywords j19140integralobservationssourcetransientx-rayanalysisbinary

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IGR J19140+098 (SIMBAD corrected name IGR J19140+0951) is a new X-ray transient, discovered by INTEGRAL during an observation of GRS 1915+015. The source presents strong variations on timescales from seconds to days. We present results of multiwavelength observations, including spectral analysis of INTEGRAL observations, and propose that IGR J19140+098 is a Galactic X-ray binary. Further classification of the source is also discussed.

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IGR J19140+098, a new INTEGRAL transient

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