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 byHIRANO 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. oFig.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 byMATTHEWS 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. oFirst reference in 1999, Proc. Star formation, ed. T. Nakamoto (Nagano): Discovery of two extreme young protostars in Barnard 1. oFig.1: <[HKM99] B1-a> (Nos B1-c, B1-d) added. Originof the Acronym: S = Created by Simbad, the CDS Database
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