Details on Acronym: [RAB2011] | |
[RAB2011] | (Roy+Ade+Bock+, 2011)= ([RAB2011a]) |
Write: | <<[RAB2011] KN>> <<[RAB2011] ICNN>> <<[RAB2011] GLL.ll+B.bb>> |
N: | 5+10+3 |
Object: | smm Clump (SIMBAD class: smmRad = Sub-Millimetric Source) |
Stat: | is completely incorporated in Simbad |
Note: | Balloon-borne Large Aperture Submillimeter Telescope (BLAST) observations of the K3-50 and IC 5146 star-forming regions. See also BLAST. |
in source: | PN K 3-50 |
in source: | IC 5146 |
Ref: | =2011ApJ...730..142R |
by | ROY A. , ADE P.A.R., BOCK J.J., BRUNT C.M., CHAPIN E.L., DEVLIN M.J., DICKER S.R., FRANCE K., GIBB A.G., GRIFFIN M., GUNDERSEN J.O., HALPERN M., HARGRAVE P.C., HUGHES D.H., KLEIN J., MARSDEN G., MARTIN P.G., MAUSKOPF P., NETTERFIELD C.B., OLMI L., PATANCHON G., REX M., SCOTT D., SEMISCH C., TRUCH M.D.P., TUCKER C., TUCKER G.S., VIERO M.P., WIEBE D.V. |
Astrophys. J., 730, 142 (2011) | |
Deconvolution of images from BLAST 2005: insight into the K3-50 and IC 5146 star-forming regions. | |
o | Table 1, col(1): <[RAB2011] KN> (Nos K1-K5) = Table 1, col(2): <BLAST JHHMMSS+DDMMSS> N=5. Table 2, col(1): <[RAB2011] ICNN> (Nos IC1-IC10) = Table 2, col(2): <BLAST JHHMMSS+DDMMSS> N=10. Fig. 10: <[RAB2011] GLL.ll+B.bb> N=3. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |
Details on Acronym: [RAB2011a] | |
[RAB2011a] | (Roy+Ade+Bock+, 2011) |
***** | Avoid the usage of [RAB2011a], prefer [RAB2011] |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |