Issue |
A&A
Volume 576, April 2015
|
|
---|---|---|
Article Number | A36 | |
Number of page(s) | 5 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/201424879 | |
Published online | 24 March 2015 |
Research Note
MAGIC observations of MWC 656, the only known Be/BH system
1
IFAE, Campus UAB
08193
Bellaterra
Spain
2
Università di Udine, and INFN Trieste, 33100
Udine,
Italy
3
INAF National Institute for Astrophysics,
00136
Rome,
Italy
4
Università di Siena, and INFN Pisa, 53100
Siena,
Italy
5
Croatian MAGIC Consortium, Rudjer Boskovic Institute, University
of Rijeka and University of Split, 10000
Zagreb,
Croatia
6
Max-Planck-Institut für Physik, 80805
München,
Germany
7
Universidad Complutense, 28040
Madrid,
Spain
8
Inst. de Astrofísica de Canarias, 38200
La Laguna, Tenerife,
Spain
9
University of Łódź, 90236
Lodz,
Poland
10
Deutsches Elektronen-Synchrotron (DESY),
15738
Zeuthen,
Germany
11
ETH Zurich, 8093
Zurich,
Switzerland
12
Universität Würzburg, 97074
Würzburg,
Germany
13
Centro de Investigaciones Energéticas, Medioambientales y
Tecnológicas, 28040
Madrid,
Spain
14
Institute of Space Sciences, 08193
Barcelona,
Spain
15
Università di Padova and INFN, 35131
Padova,
Italy
16
Technische Universität Dortmund, 44221
Dortmund,
Germany
17
Unitat de Física de les Radiacions, Departament de Física, and
CERES-IEEC, Universitat Autònoma de Barcelona, 08193
Bellaterra,
Spain
18
Universitat de Barcelona, ICC, IEEC-UB, 08028
Barcelona,
Spain
19 Japanese MAGIC Consortium, Division of Physics and
Astronomy, Kyoto University, Japan
20
Finnish MAGIC Consortium, Tuorla Observatory, University of Turku
and Department of Physics, University of Oulu, 90014
Oulun,
Finland
21
Inst. for Nucl. Research and Nucl. Energy,
1784
Sofia,
Bulgaria
22
Università di Pisa, and INFN Pisa, 56126
Pisa,
Italy
23
ICREA and Institute of Space Sciences,
08193
Barcelona,
Spain
24
Università dell’Insubria and INFN Milano Bicocca, Como, 22100
Como,
Italy
25
Now at: NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
and Department of Physics and Department of Astronomy, University of
Maryland, College
Park, MD
20742,
USA
26
Now at: École polytechnique fédérale de Lausanne
(EPFL), 1015
Lausanne,
Switzerland
27
Now at: Institut für Astro- und Teilchenphysik, Leopold-Franzens-
Universität Innsbruck, 6020
Innsbruck,
Austria
28
Now at: Finnish Centre for Astronomy with ESO
(FINCA), 20014
Turku,
Finland
29
Now at: Astrophysics Science Division,
Bhabha Atomic Research Centre,
400085
Mumbai,
India
30 Also at INAF-Trieste
31
Now at: ASTRON Netherlands Institute for Radio
Astronomy, Oude Hoogeveensedijk
4, 7991 PD
Dwingeloo, The
Netherlands
Received: 29 August 2014
Accepted: 5 February 2015
Context. MWC 656 has recently been established as the first observationally detected high-mass X-ray binary system containing a Be star and a black hole (BH). The system has been associated with a gamma-ray flaring event detected by the AGILE satellite in July 2010.
Aims. Our aim is to evaluate whether the MWC 656 gamma-ray emission extends to very high energy (VHE > 100 GeV) gamma rays.
Methods. We observed MWC 656 with the MAGIC telescopes for ~23 h during two observation periods: between May and June 2012, and in June 2013. During the last period, observations were performed contemporaneously with X-ray (XMM-Newton) and optical (STELLA) instruments.
Results. We did not detect the MWC 656 binary system at TeV energies with the MAGIC telescopes in either of the two campaigns. Upper limits (ULs) to the integral flux above 300 GeV have been set, as well as differential ULs at a level of ~5% of the Crab nebula flux. The results obtained from the MAGIC observations do not support persistent emission of VHE gamma rays from this system at a level of 2.4% the Crab flux.
Key words: astroparticle physics / binaries: general / gamma rays: stars / X-rays: binaries / stars: individual: MWC 656
© ESO, 2015
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