中文
相关论文

相关论文: A Study of the Temperature gradient in Virgo/M87 w…

200 篇论文

The high spatial resolution of the MECS experiment on board Beppo-SAX has encouraged a few scientists, including the author, to perform observations of galaxy clusters. Results from the analysis of the first few observed objects are…

天体物理学 · 物理学 2009-10-30 S. Molendi

We present hard X-ray observations of the nearby radio galaxy M87 and the core of the Virgo cluster using the Rossi X-ray Timing Explorer. These are the first hard X-ray observations of M87 not affected by contamination from the nearby…

天体物理学 · 物理学 2015-09-16 C. S. Reynolds , S. Heinz , A. C. Fabian , M. C. Begelman

We have derived azimuthally-averaged radial temperature profiles of the X-ray gas contained within 11 clusters of galaxies with redshift z=0.03-0.2 with BeppoSAX. Each of the 11 clusters have had their radial temperature profiles previously…

天体物理学 · 物理学 2009-10-31 Jimmy A. Irwin , Joel N. Bregman

At a flux limit of ~10^(-11) erg/cm2/s in the 20-100 keV band, the PDS instrument on-board BeppoSAX offers the opportunity to study the extragalactic sky with an unprecedented sensitivity. In this work we report on the results of a search…

天体物理学 · 物理学 2009-11-11 R. Landi , A. Malizia , L. Bassani

The combination of the broad band coverage and moderate spectral resolution of the LECS and MECS instruments on-board BeppoSAX allow the spectra of AGN to be studied in unprecedented detail down to 0.1 keV. We describe the calibration and…

天体物理学 · 物理学 2015-06-24 Astrid Orr , A. N. Parmar , T. Yaqoob , M. Guainazzi

The high energy experiment PDS is one of the Narrow Field Instruments aboard the X-ray astronomy satellite BeppoSAX. It covers the energy band from 15 to 300 keV. Here we report results on its in-flight performance and observations of…

天体物理学 · 物理学 2009-10-30 F. Frontera , D. Dal Fiume , E. Costa , M. Feroci , M. Orlandini , L. Nicastro , E. Palazzi , G. Zavattini , P. Giommi

We compare a very deep X-ray image of M87, at the center of the Virgo Cluster, to high-quality optical images of the low excitation emission-line gas in the same region. There are striking coincidences of detail between the two. We explore…

天体物理学 · 物理学 2009-11-10 William B. Sparks , Megan Donahue , Andres Jordan , Laura Ferrarese , Patrick Cote

We report the current status of the analysis of the MECS background using the entire dataset of the BeppoSAX Science performance Verification Phase. We have collected 360 ks of dark Earth instrumental background, 470 ks of bright Earth…

天体物理学 · 物理学 2015-06-24 L. Chiappetti , G. Cusumano , S. Del Sordo , M. C. Maccarone , T. Mineo , S. Molendi

A next-generation medium-energy gamma-ray telescope targeting the MeV range would address open questions in astrophysics regarding how extreme conditions accelerate cosmic-ray particles, produce relativistic jet outflows, and more. One…

We present results from the analysis of a BeppoSAX observation of the Centaurus Cluster. The radial metal abundance profile shows evidence of a large enhancement in the core, where Ab $>$ 1 (sol. units). The temperature map indicates that…

天体物理学 · 物理学 2009-11-07 S. Molendi , S. De Grandi , M. Guainazzi

We present results from a BeppoSAX observation of the cooling flow cluster PKS 0745-191 (z=0.1028). By performing spatially resolved spectroscopy, we find that the projected temperature profile is consistent with being constant. We can rule…

天体物理学 · 物理学 2007-05-23 Sabrina De Grandi , Silvano Molendi

In this contribution we discuss briefly a few calibration items relevant to the data analysis and present some preliminary scientific results. The discussion on instrumental topics focuses on the response matrix and Point Spread Function…

We report on a BeppoSAX Low-Energy Concentrator Spectrometer (LECS) observation of the super-soft source (SSS) CAL83. The X-ray emission in SSS is believed to arise from nuclear burning of accreted material on the surface of a white dwarf…

天体物理学 · 物理学 2007-05-23 A. N. Parmar , P. Kahabka , H. W. Hartmann , J. Heise

We report the observation of the Intra-Cluster Medium (ICM) of Abell 85 by the X-ray satellite BeppoSAX. We have both analysed the spectrum obtained in the central 8 arcmin circular region centred on the Very Steep Spectrum Radio Source…

天体物理学 · 物理学 2009-11-06 G. B. Lima Neto , V. Pislar , J. Bagchi

We present the first results of BeppoSAX observations of a small sample of low brightness FRI radio galaxies. The flux of all the targets is consistent with a thermal spectrum, as due to the presence of hot intracluster gas or galactic…

天体物理学 · 物理学 2015-06-24 E. Trussoni , F. Vagnetti , S. Massaglia , L. Feretti , P. Parma , R. Morganti , R. Fanti , P. Padovani , G. Bodo

A long ($>100,000$ seconds) observation of the bright BL Lac object PKS 2155-304 has been carried out with the Narrow Field Instruments of the BeppoSAX satellite as part of the Science Verification Phase. The source was detected between 0.1…

天体物理学 · 物理学 2007-05-23 P. Giommi et al

We present X-ray observations of two high redshift clusters of galaxies carried out with the BeppoSAX satellite. One cluster, RXJ0152.7-1357 at z = 0.83, was selected from the ROSAT Deep Cluster Survey sample, as one of the most X-ray…

天体物理学 · 物理学 2007-05-23 R. Della Ceca , R. Scaramella , I. M. Gioia , P. Rosati , F. Fiore , G. Squires

Using the Herschel PACS and SPIRE FIR/submm data, we investigate variations in the dust spectral index $\beta$ in the nearby spiral galaxy M33 at a linear resolution of 160 pc. We use an iteration method in two different approaches, single…

宇宙学与河外天体物理 · 物理学 2015-06-03 F. S. Tabatabaei , J. Braine , C. Kramer , M. Xilouris , M. Boquien , S. Verley , E. Schinnerer , D. Calzetti , F. Combes , F. Israel , C. Henkel , The HerM33es Team

We report on Cyg X-1 observations performed by the SPI telescope onboard the INTEGRAL mission and distributed over more than 6 years. We investigate the variability of the intensity and spectral shape of this peculiar source in the hard…

高能天体物理现象 · 物理学 2015-05-30 Elisabeth Jourdain , Jean-Pierre Roques , Julien Malzac

Based on mapping observations with ASCA, an unusual hot region with a spatial extent of 1 square degree was discovered between M87 and M49 at a center coordinate of R. A. = 12h 27m 36s and Dec. = $9^\circ18'$ (J2000). The X-ray emission…

‹ 上一页 1 2 3 10 下一页 ›