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G320.4-1.2

  • Common Name: MSH 15-52, RCW 89
  • Distance: 4.2kpc( Caswell et al., 1975 )
  • Position of Central Source (J2000): ( 15 13 55.6, -59 08 09.5 )
  • X-ray size: 18'x11'
  • Description:
Not available754/work/tr2.jpg
RadioX-Ray


Summary of Chandra Observations

SequenceObs. IDDetectors UsedExposure uf
(ks)
Exposure f
(ks)
Date
Observed
Aimpoint (J2000)
(RA, Dec)
500050 754 ACIS-012379 19.0 18.9 2000-08-14 ( 15 13 55.6, -59 08 08.9 )


Exposureuf => Exposure time of unfiltered event file
Exposuref => Exposure time of filtered event file
  • Observed with ACIS-I chips.
  • No CTI correction is applied.

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.)
754 15.5 MB 11.3 MB 5.3 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)
Pulsar and PWN 0.3 - 10.0 1.067e+05 5.635e+00 8.86e-11 1.53e-10 3.22e+35
0.3 - 2.1 5.360e+04 2.830e+00 1.34e-11 7.19e-11 1.51e+35
2.1 - 10.0 5.347e+04 2.823e+00 7.54e-11 8.13e-11 1.71e+35
RCW 89 0.3 - 10.0 4.873e+04 2.573e+00 2.22e-11 3.01e-10 6.34e+35
0.3 - 2.1 3.983e+04 2.103e+00 9.97e-12 2.88e-10 6.05e+35
2.1 - 10.0 8.979e+03 4.741e-01 1.22e-11 1.35e-11 2.84e+34


NH = 1.0(1022 cm-2) Assumed distance: 4.2kpc ( Caswell et al., 1975 )

Chandra Images



Chandra Spectra



Other Wavelengths



Compact Sources

Obs. IDPosition (J2000)SizeNet CountCount rateNote
754
( 15 12 44.9, -59 05 40.5 ) < 11.9" 133.0 6.99e-03
( 15 12 55.9, -59 06 36.2 ) < 7.9" 31.7 1.67e-03
( 15 13 08.7, -59 15 05.8 ) < 11.0" 40.7 2.14e-03
( 15 13 41.7, -59 11 44.9 ) < 3.0" 172.0 9.03e-03
( 15 13 56.3, -59 15 29.0 ) < 6.6" 23.0 1.21e-03
( 15 14 00.2, -59 12 38.0 ) < 3.1" 43.1 2.26e-03
( 15 14 05.4, -59 14 38.5 ) < 5.9" 21.8 1.15e-03
( 15 14 32.3, -59 08 09.0 ) < 4.1" 28.4 1.49e-03
( 15 14 49.0, -59 08 19.0 ) < 5.8" 30.3 1.59e-03
( 15 14 52.8, -59 08 14.6 ) < 5.9" 17.5 9.19e-04


  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



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Chandra Supernova Remnant Catalog
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