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G011.2-00.3

  • Distance: 5kpc( Green et al., 1988 )
  • Position of Central Source (J2000): ( 18 11 29.3, -19 25 27.1 )
  • X-ray size: 4.5'x4.4'
  • Description: Circular outer shell with central source
radio/g11.2-0.3_21cm_ohgeo.fits.small.jpg780/work/tr2.jpg
RadioX-Ray


Summary of Chandra Observations

SequenceObs. IDDetectors UsedExposure uf
(ks)		Exposure f
(ks)		Date
Observed		Aimpoint (J2000)
(RA, Dec)
500076 780 ACIS-235678 21.1 19.4 2000-08-06 ( 18 11 29.4, -19 25 25.0 )


Exposureuf => Exposure time of unfiltered event file
Exposuref => Exposure time of filtered event file
  • The whole remnant is covered by chip ACIS-S3(CCD_ID=7)

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.)
780 14.0 MB 7.4 MB 5.2 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 9.272e+04 4.791e+00 3.26e-11 3.98e-09 1.19e+37
0.3 - 2.1 7.100e+04 3.669e+00 1.47e-11 3.95e-09 1.18e+37
2.1 - 10.0 2.202e+04 1.138e+00 1.80e-11 3.00e-11 8.94e+34


NH = 3.1(1022 cm-2) Assumed distance: 5kpc ( Green et al., 1988 )

Chandra Images



Chandra Spectra



Other Wavelengths



Compact Sources

Obs. IDPosition (J2000)SizeNet CountCount rateNote
780
( 18 10 32.9, -19 17 53.3 ) < 35.0" 114.0 5.40e-03
( 18 10 49.2, -19 31 25.0 ) < 16.3" 26.2 1.24e-03
( 18 10 56.9, -19 34 00.7 ) < 15.7" 63.4 3.00e-03
( 18 10 59.6, -19 22 33.7 ) < 8.7" 27.2 1.29e-03
( 18 11 13.6, -19 33 42.0 ) < 9.0" 267.0 1.26e-02
( 18 11 17.1, -19 22 23.1 ) < 5.9" 17.6 8.34e-04
( 18 11 19.2, -19 26 33.1 ) < 5.9" 97.2 4.60e-03
( 18 11 19.3, -19 29 36.1 ) < 5.9" 16.6 7.86e-04
( 18 11 38.6, -19 24 26.0 ) < 5.6" 59.3 2.81e-03
( 18 11 40.6, -19 21 54.6 ) < 4.6" 53.2 2.52e-03
( 18 11 41.9, -19 28 15.4 ) < 2.3" 41.3 1.96e-03
( 18 11 42.1, -19 19 41.0 ) < 8.8" 55.8 2.64e-03
( 18 11 42.4, -19 18 42.9 ) < 12.6" 25.9 1.23e-03


  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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