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Chandra Images for G33.6+0.1
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G33.6+0.1

  • Common Name: Kes 79
  • Distance: 7kpc(Sun et al 2004)
  • Position of Central Source (J2000): ( 18 52 38.6, 00 40 19.8 )
  • X-ray size: 10'x8'
  • Description: mixed morphology with CCO
Not available1982/work/tr2.jpg
RadioX-Ray


Summary of Chandra Observations

SequenceObs. IDDetectors UsedExposure uf
(ks)
Exposure f
(ks)
Date
Observed
Aimpoint (J2000)
(RA, Dec)
500159 1982 ACIS-012367 29.6 29.4 2001-07-31 ( 18 52 39.0, 00 40 00.0 )


Exposureuf => Exposure time of unfiltered event file
Exposuref => Exposure time of filtered event file

    Chandra Event File

    Click left mouse button on hyperlink below to download file
    Obs. IDEvent 2 FITS File
    (un-filtered)
    Event 2 FITS File
    (filtered)
    AUX file
    (asol, badpix etc.)
    1982 12.4 MB 6.6 MB 7.9 MB


    Chandra Counts and Fluxes

    RegionEnergy Range
    (keV)
    Signal
    (counts)
    Rate
    (counts s-1)
    FabsX
    (ergs cm-2s-1)
    FX
    (ergs cm-2s-1)
    LX
    (ergs s-1)
    total 0.3 - 10.0 4.820e+04 1.638e+00 1.02e-11 1.74e-10 1.02e+36
    0.3 - 2.1 4.253e+04 1.446e+00 6.38e-12 1.69e-10 9.87e+35
    2.1 - 10.0 5.772e+03 1.962e-01 3.88e-12 5.08e-12 2.97e+34


    NH = 1.5(1022 cm-2) Assumed distance: 7kpc (Sun et al 2004)

    Chandra Images



    Chandra Spectra



    Other Wavelengths



    Compact Sources

    Obs. IDPosition (J2000)SizeNet CountCount rateNote
    1982
    ( 18 52 05.3, 00 42 08.0 ) < 11.6" 54.7 1.85e-03
    ( 18 52 12.9, 00 43 28.3 ) < 8.2" 49.5 1.67e-03
    ( 18 52 13.0, 00 37 37.5 ) < 7.3" 75.3 2.55e-03
    ( 18 52 29.5, 00 51 08.6 ) < 23.0" 48.2 1.63e-03
    ( 18 52 41.6, 00 47 00.5 ) < 7.1" 76.8 2.60e-03
    ( 18 52 44.4, 00 29 54.0 ) < 20.7" 53.8 1.82e-03
    ( 18 53 02.9, 00 44 22.3 ) < 9.2" 69.9 2.36e-03
    ( 18 53 11.0, 00 41 24.7 ) < 12.8" 54.5 1.84e-03
    ( 18 53 17.0, 00 27 47.9 ) < 36.4" 38.9 1.32e-03
    ( 18 53 30.3, 00 33 52.0 ) < 36.0" 216.0 7.30e-03
    ( 18 53 38.5, 00 33 56.0 ) < 41.1" 2330.0 7.88e-02


    1. This list is not complete. Sources are obvious and usually within or close to the remnant. The size refers to the appearance of the source and can be larger for off-axis sources.


    References



    line
    Chandra Supernova Remnant Catalog
    Main Page | Galactic SNR | Magellanic Cloud SNR
    True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR