2006ApJ...644L.171N

Query : 2006ApJ...644L.171N

2006ApJ...644L.171N - Astrophys. J., 644, L171-L174 (2006/June-3)

Far-ultraviolet spectral images of the Vela supernova remnant.

NISHIKIDA K., EDELSTEIN J., KORPELA E.J., SANKRIT R., FEUERSTEIN W.M., MIN K.W., SHINN J.-H., LEE D.-H., YUK I.-S., JIN H. and SEON K.-I.

Abstract (from CDS):

We present far-ultraviolet (FUV) spectral imaging observations of the Vela supernova remnant (SNR) obtained with the SPEAR/FIMS instrument. The Vela SNR extends ∼8° in the FUV, and its global spectra are dominated by shock-induced emission lines. We find that the global FUV line luminosities can exceed the 0.1-2.5 keV soft X-ray luminosity by an order of magnitude. The global O VI:C III ratio shows that the Vela SNR has a relatively large fraction of slower shocks compared with the Cygnus Loop.

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Journal keyword(s): ISM: individual (Vela supernova remnant) - ISM: Supernova Remnants - Ultraviolet: ISM

Simbad objects: 10

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Number of rows : 10
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 [AET95] E X 07 58 07 -44 38.0           ~ 5 0
2 [AET95] F X 08 07 51 -41 29.5           ~ 4 0
3 NAME Vela X Psr 08 33 08.880 -45 11 24.36           ~ 302 1
4 NAME Vela SNR 08 34.0 -45 50           ~ 1331 2
5 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2446 1
6 [AET95] A X 08 57 55 -41 49.4           ~ 9 0
7 [AET95] D Rad 09 01 10 -45 31.7           ~ 12 0
8 [AET95] B X 09 03 02 -43 33.1           ~ 6 0
9 [AET95] C X 09 05 40 -44 29.4           ~ 5 0
10 NAME Cyg Loop SNR 20 51.0 +30 40           ~ 964 0

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