1999AJ....117.1387C


Query : 1999AJ....117.1387C

1999AJ....117.1387C - Astron. J., 117, 1387-1391 (1999/March-0)

No water masers associated with supernova remnants.

CLAUSSEN M.J., GOSS W.M., FRAIL D.A. and SETA M.

Abstract (from CDS):

We have used the Very Large Array to search for water masers in the three supernova remnants W28, W44, and IC 443. Only one candidate maser was detected, in W44. Follow-up observations using the VLA at 1612 MHz demonstrate that the water maser in W44 is likely associated with a late-type star and not a shock in the supernova remnant. The nondetection of water masers toward shocked regions in these supernova remnants places constraints on the postshock density and is consistent with the density determined by molecular observations and the limits from 1720 MHz OH maser pumping.

Abstract Copyright: ∼

Journal keyword(s): ISM: individual (W28, W44, IC 443) - ISM: Masers - ISM: Supernova Remnants

Nomenclature: Table 6: [CGF99] W44 Maser N=1.

CDS comments: [CGF99] W44 Maser has been previously discovered by Seta+ 1997 (publication not in SIMBAD).

Simbad objects: 12

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Number of rows : 12
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 IC 443G PoC 06 16 43.4 +22 32 24           ~ 35 1
2 [HDS86] IC 443A PoC 06 16 56.0 +22 23 48           ~ 10 0
3 IC 443 SNR 06 17 00.0000000 +22 34 11.998901           ~ 1314 1
4 IC 443B Cld 06 17 16 +22 25.7           ~ 25 1
5 IC 443C PoC 06 17 44.2 +22 21 49           ~ 32 0
6 IC 443D PoC 06 17 53.2 +22 23 50           ~ 9 1
7 IC 443E PoC 06 18.2 +22 40           ~ 8 0
8 SNR G006.4-00.1 SNR 18 00 31.2011719 -23 25 48.001099           ~ 782 1
9 [CGF99] W44 Maser Mas 18 56 09.03 +01 28 35.8           ~ 1 0
10 SNR G034.6-00.5 SNR 18 56 10.650 +01 13 21.30           ~ 1034 2
11 [HDS86] IC 443H PoC ~ ~           ~ 5 0
12 IC 443F PoC ~ ~           ~ 8 0

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