J/ApJ/665/1297     X-ray sources around G12.82-0.02          (Helfand+, 2007)

Discovery of the putative pulsar and wind nebula associated with the TeV gamma-ray source HESS J1813-178. Helfand D.J., Gotthelf E.V., Halpern J.P., Camilo F., Semler D.R., Becker R.H., White R.L. <Astrophys. J., 665, 1297-1303 (2007)> =2007ApJ...665.1297H 2007ApJ...665.1297H
ADC_Keywords: X-ray sources ; Photometry Keywords: pulsars: general - stars: individual (CXOU J181335.1-174957, G12.82-0.02) - stars: neutron - supernova remnants - X-rays: stars Abstract: We present a Chandra X-ray observation of G12.82-0.02, a shell-like radio supernova remnant coincident with the TeV gamma-ray source HESS J1813-178. We resolve the X-ray emission from the colocated Advanced Satellite for Cosmology and Astrophysics (ASCA) source into a point source surrounded by structured diffuse emission that fills the interior of the radio shell. The morphology of the diffuse emission strongly resembles that of a pulsar wind nebula. Description: A 30ks X-ray observation of SNR G12.82-0.02 was obtained on 2006 September 15 UT using the Chandra X-Ray Observatory. Data were collected with the Advanced CCD Imaging Spectrometer (ACIS) in the focal plane, operating in the nominal full-frame TIMED/VFAINT exposure mode. This detector is sensitive to X-rays in the 0.3-12.0keV energy range. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 54 75 Sources in CHANDRA ACIS-I ObsID 6685 -------------------------------------------------------------------------------- See also: B/chandra : The Chandra Archive Log (CXC, 1999-) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I2 --- [HGH2007] Sequential number (1) 3 A1 --- n_[HGH2007] [c] Note on [HGH2007] (1) 5- 6 I2 h RAh Right ascension (J2000) 8- 9 I2 min RAm Right ascension (J2000) 11- 16 F6.3 s RAs Right ascension (J2000) 18 A1 --- DE- Declination sign (J2000) 19- 20 I2 deg DEd Declination (J2000) 22- 23 I2 arcmin DEm Declination (J2000) 25- 29 F5.2 arcsec DEs Declination (J2000) 31- 35 F5.1 ct Counts X-ray counts (0.3-10keV) 37- 40 F4.1 ct e_Counts rms uncertainty on Counts 42- 46 F5.2 --- HR Hardness ratio (2) 48 A1 --- l_Rmag Limit flag on Rmag 49- 53 F5.2 mag Rmag ? R magnitude (3) 54 A1 --- u_Rmag Uncertainty flag on Rmag due to blending -------------------------------------------------------------------------------- Note (1): the note (c) indicates that the USNO-B1.0 catalog counterpart was used as an astrometric calibrator. Note (2): Hardness ratio defined as HR=(Nh-Ns)/(Nh+Ns), where Ns and Nh are the counts measured in the 0.3-2 and 2-10keV energy band, respectively. Note (3): Blank indicate that a probable optical counterpart exists, but not measured due to blending. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 06-Sep-2009
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