Details on Acronym: [HKM99] | |
[HKM99] | (Hirano+Kamazaki+Mikami+, 1999) |
Write: | <<[HKM99] B1-a>> <<[HKM99] B1-aW>> <<[HKM99] B1-IRS>> |
N: | 4+2+1 |
Object: | Part of Cloud (SIMBAD class: PartofCloud = Part of Cloud) |
Stat: | is completely incorporated in Simbad |
Note: | N=4 ammonia condensations 'B1-a' to 'B1-d' in Barnard 1 cloud. N=2 smm peaks in B1-b condensation 'B1-bN' and 'B1-bS'. |
in source: | Barnard 1 |
Ref: | =1999sf99..R....181H |
by | HIRANO N. , KAMAZAKI T., MIKAMI H., OHASHI N., UMEMOTO T. |
Proc. Star Formation 1999, 181-182 (1999) | |
Discovery of two extreme young protostars in Barnard 1. | |
o | Fig.1: <[HKM99] B1-a> (Nos B1-a, B1-b), <[HKM99] B1-bW> (Nos B1-bN, B1-bS), <[HKM99] B1-IRS> N=1. |
Ref: | =2002ApJ...574..822M |
by | MATTHEWS B.C. , WILSON C.D. |
Astrophys. J., 574, 822-833 (2002) | |
Magnetic fields in star-forming molecular clouds. V. Submillimeter polarization of the Barnard 1 dark cloud. | |
o | First reference in 1999, Proc. Star formation, ed. T. Nakamoto (Nagano): Discovery of two extreme young protostars in Barnard 1. |
o | Fig.1: <[HKM99] B1-a> (Nos B1-c, B1-d) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |