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We present a new sensitive 2675 MHz radio continuum map of the Cygnus Loop, which is used in conjunction with 408 MHz, 863 MHz and 1420 MHz maps from both the Effelsberg 100-m telescope and the DRAO Synthesis Telescope for a spectral…

天体物理学 · 物理学 2009-11-10 B. Uyaniker , W. Reich , A. Yar-Uyaniker , E. Fuerst

A three bright X-ray non-target sources are detected in the field of the seyfert 1 galaxy MKN 205. These sources are classified as optically Early-type galaxy, BLAGN, and NELG (NED, SIMBAD, and AXIS). The spectrum analysis is made for these…

高能天体物理现象 · 物理学 2019-11-11 B. Korany

Circinus X-1 is a neutron-star-accreting X-ray binary in a wide (P$_{\rm orb}$ = 16.6 d), eccentric orbit. After two years of relatively low X-ray luminosity, in May 2010 Circinus X-1 went into outburst, reaching 0.4 Crab flux. This…

高能天体物理现象 · 物理学 2015-06-04 A. D'Aì , E. Bozzo , A. Papitto , R. Iaria , T. Di Salvo , L. Burderi , A. Riggio , E. Egron , N. R. Robba

We consider a model in which massive stars form in a self-gravitating accretion disk around an active galactic nucleus (AGN). These stars may evolve and collapse to form compact objects on a time scale shorter than the accretion time, thus…

天体物理学 · 物理学 2008-11-26 Guenter Sigl , Jeremy Schnittman , Alessandra Buonanno

We present results from the zeroth-order imaging of a Chandra HETGS observation of the nearby Seyfert 2 galaxy Circinus. Twelve X-ray sources were detected in the ACIS-S image of the galaxy, embedded in diffuse X-ray emission. The latter…

天体物理学 · 物理学 2009-10-31 R. M. Sambruna , W. N. Brandt , G. Chartas , H. Netzer , S. Kaspi , G. P. Garmire , J. A. Nousek , K. A. Weaver

We present the results of the optical identifications of a set of X-ray sources from the all-sky surveys of INTEGRAL and SWIFT observatories. Optical data were obtained with Russian-Turkish 1.5-m Telescope (RTT150). Nine X-ray sources were…

We report the detection of six discrete, low-luminosity (Lx < 10^33 erg/s) X-ray sources, located within 12 arcsec of the center of the collapsed-core globular cluster M30 (NGC 7099), and a total of 13 sources within the half-mass radius,…

We studied the energy spectrum and the large-scale fluctuation of the X-ray background with the ASCA GIS based on the ASCA MSS and LSS observations. A total of 91 fields with Galactic latitude |b|>10 deg were selected with a sky coverage of…

We present results of a comprehensive study of the distribution of absorption dips with orbital phase in Cygnus X-1. Firstly, the distribution was obtained using archival data from all major X-ray observatories and corrected for the…

天体物理学 · 物理学 2009-10-31 M. Balucinska-Church , M. J. Church , P. A. Charles , F. Nagase , J. LaSala , R. Barnard

We observed the nearby galaxy M~51 (NGC 5194) with BeppoSAX. The X-ray properties of the nucleus below 10 keV are almost the same as the ASCA results regarding the hard component and the neutral Fe K$\alpha$ line, but the intensity is about…

天体物理学 · 物理学 2009-11-06 Yasushi Fukazawa , Naoko Iyomoto , Aya Kubota , Yukari Matsumoto , Kazuo Makishima

We report the results of XMM-Newton observations for an especially luminous supersoft X-ray source (SSS) with bolometric luminosity of 10^39 erg/s in the spiral galaxy NGC 300. The source was detected as a SSS in 1992 and disappeared in…

天体物理学 · 物理学 2009-11-07 A. K. H. Kong , R. Di Stefano

We present Chandra and XMM-Newton observations of the composite star-forming/Seyfert galaxy IRAS20051-1117. The X-ray imaging and spectral properties reveal the presence of an active nucleus. The Chandra image shows a strong nuclear point…

天体物理学 · 物理学 2009-11-10 I. Georgantopoulos , I. Papadakis , A. Zezas , M. J. Ward

Aims. We investigate observations of the X-ray binary Cygnus X-1 with unusually high hardness and low flux. In particular, we study the characteristic frequencies seen in the PDS and the hardness-flux correlation within and between these…

天体物理学 · 物理学 2009-02-25 M. Axelsson , L. Hjalmarsdotter , L. Borgonovo , S. Larsson

We analyse the aperiodic flaring features, also known as shots, observed in Cyg X-1 in the 0.1-80 keV energy band using a 6.39 ks simultaneous observation with AstroSat and NICER. We detect 49 simultaneous shots in the soft and hard X-ray…

高能天体物理现象 · 物理学 2022-04-06 Yash Bhargava , Nandini Hazra , A. R. Rao , Ranjeev Misra , Dipankar Bhattacharya , Jayashree Roy , Md. Shah Alam

We present the results of a 200 ks Chandra observation of part of the Groth Strip region, using the ACIS-I instrument. We present a relatively simple method for the detection of point-sources and calculation of limiting sensitivities, which…

X-ray observations unveiled the existence of enigmatic point-like sources at the centre of young supernova remnants (SNRs). These sources, dubbed Central Compact Objects (CCOs), are thought to be neutron stars formed by the supernova…

天体物理学 · 物理学 2009-11-13 R. P. Mignani , S. Zaggia , A. De Luca , R. Perna , N. Bassan , P. A. Caraveo

The hard X-ray sensitivity and arcminute position accuracy of the recently launched International Gamma-Ray Laboratory (INTEGRAL) has lead to the (re-)discovery of a class of heavily absorbed hard X-ray sources lying in the Galactic plane.…

天体物理学 · 物理学 2009-11-07 J. Rodriguez , J. A. Tomsick , L. Foschini , R. Walter , A. Goldwurm , S. Corbel , P. Kaaret

We present results of monitoring observations of the micro-quasars CygnusX-1 and Cygnus X-3 at 0.61 and 1.28 GHz. The observations were performed with Giant Meter-wave Radio Telescope, GMRT, between 2003 June and 2005 January. Variable,…

天体物理学 · 物理学 2009-11-11 M. Pandey , A. P. Rao , G. G. Pooley , P. Durouchoux , R. K. Manchanda , C. H. Ishwara-Chandra

We present the preliminary results of the observational campaign performed in 2003 to study the Galactic Nucleus with INTEGRAL. The mosaicked images obtained with the IBIS/ISGRI coded aperture instrument in the energy range above 20 keV,…

The anomalous X-ray pulsars (AXPs) represent a growing class of neutron stars discovered at X-ray energies. While the nature of their multi-wavelength emission mechanism is still under debate, evidence has been recently accumulating in…

天体物理学 · 物理学 2009-11-10 Samar Safi-Harb , Jennifer West