Details on Acronym: IRS | |
IRS | (IR Source) |
***** | Avoid the usage of IRS, prefer SSV |
Origin | of the Acronym: L = Found in the literature |
Details on Acronym: SSV | |
SSV | (Strom+Strom+Vrba)= (IRS) |
Write: | <<SSV LDN 1630 NNW>> <<SSV LDN 1551 NA>> <<SSV LDN 1517 NN>> |
N: | 70+6+13 |
Object: | (IR) (SIMBAD class: Infrared = Infra-Red Source) |
Stat: | is completely incorporated in Simbad |
Note: | See the remark for VSSG 'SSV LDN 1551 5' is often found in the literature as 'LDN 1551 IRS 5' with 2 components 5A and 5B, also found in the literature respectively as 5N and 5S. |
in source: | LDN 1630 |
in source: | LDN 1551 |
in source: | LDN 1517 |
Ref: | =1976AJ.....81..308S |
by | STROM K.M. , STROM S.E., VRBA F.J. |
Astron. J., 81, 308-313 (1976) | |
Infrared surveys of dark-cloud complexes. I. The Lynds 1630 dark cloud. | |
o | <SSV LDN 1630 NN> (Nos 1-70) |
Ref: | =1976AJ.....81..320S |
by | STROM K.M. , STROM S.E., VRBA F.J. |
Astron. J., 81, 320-322 (1976) | |
Infrared surveys of dark- cloud complexes. IV. The Lynds 1517 and Lynds 1551 clouds. | |
o | Table I: <SSV LDN 1551 N> (Nos 1-6), Table II: <SSV LDN 1517 NN> (Nos 1-13). 'SSV LDN 1551 5' = <NAME LDN 1551 IRS 5> |
Ref: | =1997ApJ...484L.157L |
by | LOONEY L.W. , MUNDY L.G., WELCH W.J. |
Astrophys. J., 484, 157-160 (1997) | |
High-resolution λ= 2.7 millimeter observations of L1551 IRS 5. | |
o | p. 158: <SSV LDN 1551 5A>, SSV LDN 1551 5B> |
Ref: | =1997A&A...324..263D |
by | DAVIS C.J. , RAY T.P., EISLOEFFEL J., CORCORAN D. |
Astron. Astrophys., 324, 263-275 (1997) | |
Near-IR imaging of the molecular outflows in HH 24-26, L 1634 (HH 240-241), L 1660 (HH 72) and RNO 15-FIR. | |
o | Table 5 : IRAS 03282 = 03282+3035, 21334 = 21334+5039 |
o | Fig.1: <SSV LDN 1630 NNW> (Nos 63E, 63W). Table 2: <HH NNN> (No. 241). |