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| Query : 2002AstL...28..217S |
2002AstL...28..217S - Astron. Lett., 28, 217-222 (2002)
A possible formation mechanism of the asymmetry in the H2O maser emission line.
SILANT'EV N.A., LEKHT E.E., MENDOZA-TORRES J.E. and TOLMACHEV A.M.
Journal keyword(s):
Simbad objects: 6
| Number of rows : 6 |
| 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 | NGC 2071 | RNe | 05 47 10 | +00 18.0 | ~ | 661 | 1 | |||||
| 2 | LBN 196.49-01.60 | HII | 06 14 38.29 | +13 49 41.0 | ~ | 169 | 1 | |||||
| 3 | OH 043.796-00.127 | Mas | 19 11 53.9868 | +09 35 50.325 | ~ | 89 | 0 | |||||
| 4 | [KCW94] 069.540-00.975 | HII | 20 10 08.95 | +31 31 35.4 | ~ | 168 | 1 | |||||
| 5 | IRAS 20081+3122 | Y*O | 20 10 09.036 | +31 31 34.14 | ~ | 172 | 0 | |||||
| 6 | Onsala 1 | cor | 20 10 09.2036 | +31 31 36.090 | ~ | 194 | 0 |
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