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A&A 433, L45-L48 (2005)
DOI: 10.1051/0004-6361:200500023
Letter
INTEGRAL observation of V 0332+53 in outburst
I. Kreykenbohm1, 2, N. Mowlavi2, 3, N. Produit2, 3, S. Soldi2, 3, R. Walter2, 3, P. Dubath2, 3, P. Lubinski4, 2, M. Türler2, 3, W. Coburn5, A. Santangelo1, R. E. Rothschild5 and R. Staubert11 Institut für Astronomie und Astrophysik - Astronomie, Sand 1, 72076 Tübingen, Germany
2 INTEGRAL Science Data Centre, 16 Ch. d'Écogia, 1290 Versoix, Switzerland
e-mail: Ingo.Kreykenbohm@obs.unige.ch
3 Observatoire de Genève, Chemin des Maillettes 51, 1290 Sauverny, Switzerland
4 N. Copernicus Astronomical Center, Bartycka 18, Warsaw 00-716, Poland
5 Space Sciences Laboratory, University of California, Berkeley, Berkeley, CA, 94702-7450, USA
(Received 18 January 2005 / Accepted 9 February 2005)
Abstract
We present the analysis of a 100 ks INTEGRAL
(3-100
) observation of the transient X-ray pulsar V 0332+53in
outburst. The source is pulsating at
s with a clear double pulse from
6
to 60
. The average flux was ~550 mCrab between
20
and 60
. We modeled the broad band continuum from
5
to 100
with a power-law modified by an exponential cut
off. We observe three cyclotron lines: the fundamental line at
24.9
+0.1-0.1
, the first harmonic at
50.5
+0.1-0.1
as well as the second harmonic at
71.7
+0.7-0.8
, thus confirming the discovery of the harmonic lines by Coburn et al. (2005) in RXTEdata.
Key words: X-rays: stars -- stars: flare -- stars: pulsars: individual: V0332+53 -- stars: magnetic fields
SIMBAD Objects
© ESO 2005
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