The Experts below are selected from a list of 180 Experts worldwide ranked by ideXlab platform

Albert K. H. Kong - One of the best experts on this subject based on the ideXlab platform.

  • Erratum: “A Potential Supernova Remnant-X-Ray Binary Association in M31” (ApJ, 634, 365 [2005])
    The Astrophysical Journal, 2007
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/Optical/Radio supernova remnant DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveals a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low-mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently-available X-ray and optical data show no evidence that the XRB is high-mass. If the XRB is low-mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.Comment: 30 pages, 3 tables, 11 figures, accepted for publication in Ap

  • A potential supernova remnant-X-ray Binary Association in M31
    The Astrophysical Journal, 2005
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/optical/radio supernova remnant (SNR) DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveal a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently available X-ray and optical data show no evidence that the XRB is high mass. If the XRB is low mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.

Benjamin F. Williams - One of the best experts on this subject based on the ideXlab platform.

  • Erratum: “A Potential Supernova Remnant-X-Ray Binary Association in M31” (ApJ, 634, 365 [2005])
    The Astrophysical Journal, 2007
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/Optical/Radio supernova remnant DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveals a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low-mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently-available X-ray and optical data show no evidence that the XRB is high-mass. If the XRB is low-mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.Comment: 30 pages, 3 tables, 11 figures, accepted for publication in Ap

  • A potential supernova remnant-X-ray Binary Association in M31
    The Astrophysical Journal, 2005
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/optical/radio supernova remnant (SNR) DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveal a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently available X-ray and optical data show no evidence that the XRB is high mass. If the XRB is low mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.

Michael R. Garcia - One of the best experts on this subject based on the ideXlab platform.

  • Erratum: “A Potential Supernova Remnant-X-Ray Binary Association in M31” (ApJ, 634, 365 [2005])
    The Astrophysical Journal, 2007
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/Optical/Radio supernova remnant DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveals a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low-mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently-available X-ray and optical data show no evidence that the XRB is high-mass. If the XRB is low-mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.Comment: 30 pages, 3 tables, 11 figures, accepted for publication in Ap

  • A potential supernova remnant-X-ray Binary Association in M31
    The Astrophysical Journal, 2005
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/optical/radio supernova remnant (SNR) DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveal a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently available X-ray and optical data show no evidence that the XRB is high mass. If the XRB is low mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.

J. P. Osborne - One of the best experts on this subject based on the ideXlab platform.

  • Erratum: “A Potential Supernova Remnant-X-Ray Binary Association in M31” (ApJ, 634, 365 [2005])
    The Astrophysical Journal, 2007
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/Optical/Radio supernova remnant DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveals a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low-mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently-available X-ray and optical data show no evidence that the XRB is high-mass. If the XRB is low-mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.Comment: 30 pages, 3 tables, 11 figures, accepted for publication in Ap

  • A potential supernova remnant-X-ray Binary Association in M31
    The Astrophysical Journal, 2005
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/optical/radio supernova remnant (SNR) DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveal a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently available X-ray and optical data show no evidence that the XRB is high mass. If the XRB is low mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.

Robin Barnard - One of the best experts on this subject based on the ideXlab platform.

  • Erratum: “A Potential Supernova Remnant-X-Ray Binary Association in M31” (ApJ, 634, 365 [2005])
    The Astrophysical Journal, 2007
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/Optical/Radio supernova remnant DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveals a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low-mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently-available X-ray and optical data show no evidence that the XRB is high-mass. If the XRB is low-mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.Comment: 30 pages, 3 tables, 11 figures, accepted for publication in Ap

  • A potential supernova remnant-X-ray Binary Association in M31
    The Astrophysical Journal, 2005
    Co-Authors: Benjamin F. Williams, Robin Barnard, Michael R. Garcia, Ulrich Kolb, J. P. Osborne, Albert K. H. Kong
    Abstract:

    The well-studied X-ray/optical/radio supernova remnant (SNR) DDB 1-15 (CXOM31 J004327.8+411829; r3-63) in M31 has been investigated with archival XMM-Newton and Chandra observations. The timing data from XMM-Newton reveal a power density spectrum (PDS) characteristic of accreting compact objects in X-ray binaries (XRBs). The PDS shows features typical of Roche lobe overflow accretion, hinting that the XRB is low mass. The Chandra observations resolve the SNR into a shell and show a variable count rate at the 94% confidence level in the northwest quadrant. Together, these XMM-Newton and Chandra data suggest that there is an XRB in the SNR r3-63 and that the XRB is located in the northwestern portion of the SNR. The currently available X-ray and optical data show no evidence that the XRB is high mass. If the XRB is low mass, r3-63 would be the first SNR found to contain a low-mass X-ray Binary.