The broad-band spectrum of Cyg X-2 with INTEGRAL

نویسندگان

  • G. Lavagetto
  • M. van der Klis
چکیده

We study the broad band (3-100 keV) spectrum of Cygnus X–2 with INTEGRAL. We find that the spectrum is well fitted by a Comptonized component with a seed-photons temperature of ∼ 1 keV, an electron temperature of ∼ 3 keV and an optical depth τ ∼ 8. Assuming spherical geometry, the radius of the seed-photons emitting region is ∼ 17 km. The source shows no hard X-ray emission; it was detected only at a 3σ level above 40 keV. We also analyzed public ISGRI data of Cyg X–2 to investigate the presence of a hard X–ray component. We report the possible presence of hard X-ray emission in one data set.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

ar X iv : a st ro - p h / 98 02 07 8 v 1 6 F eb 1 99 8 1 High energy properties of X – ray sources observed with BeppoSAX

We report on highlight results on celestial sources observed in the high energy band (> 20 keV) with BeppoSAX . In particular we review the spectral properties of sources that belong to different classes of objects, i.e., stellar coronae (Algol), supernova remnants (Cas A), low mass X–ray binaries (Cygnus X–2 and the X–ray burster GS1826–238), black hole candidates (Cygnus X–1) and Active Galac...

متن کامل

The X-ray spectral evolution of Cyg X–2 in the framework of bulk Comptonization

Context. The interplay of thermal and bulk motion Comptonization to explain the spectral evolution of neutron star LMXBs including transient hard X-ray tails is gaining a strong theoretical and observational support. The last momentum has been given by the advent of a new XSPEC Comptonization model, COMPTB, which includes thermal and bulk Comptonization. Aims. We used COMPTB to investigate the ...

متن کامل

An intense state of hard X-ray emission of Cyg X-1 observed by INTEGRAL coincident with TeV measurements

Aims. We present INTEGRAL light curves and spectra of the black-hole binary Cyg X-1 during a bright event that occurred in 2006 September, and which was simultaneous with a detection at 0.15–1 TeV energies by the MAGIC telescope. Methods. We analyse the hard X-ray emission from 18 to 700 keV with the INTEGRAL data taken on 2006 September 24–26 by the IBIS and SPI instruments. These data are sup...

متن کامل

First IBIS results on the high energy emission of Cyg X - 2 ⋆

The bright low-mass X-ray binary Cyg X-2 was in the field of view of the IBIS telescope during the early Cygnus region observations, executed during the INTEGRAL Performance Verification Phase. The data presented are spanning about one week and cover the rising edge of one of the two peaks of the ≈ 82 day cycle of the Cyg X-2 light curve. The IBIS data in the energy range 20-40 keV exhibit flux...

متن کامل

ar X iv : a st ro - p h / 98 10 13 9 v 1 8 O ct 1 99 8 RXTE Observations of Cygnus X - 1 Broad - Band Spectra and High - Resolution Timing

We present results from a 20 ksec RXTE observation of the black hole candidate Cyg X-1. We apply self-consistent accretion disk corona models to these hard state data and show that Comptonization in a spherical corona irradiated by soft photons from an exterior cold disk is able to successfully model the spectrum. We also present the power spectrum, the coherence function, and the time lags for...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2005