.
Details on Acronym: MH
MH (?) ***** Avoid the usage of MH, prefer [WBK2005] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: SMM
SMM (SubMilliMeter source) ***** Avoid the usage of SMM, prefer [WBK2005] Originof the Acronym: A = Assigned by the author(s)
Details on Acronym: [WBK2005]
[WBK2005] (Walawender+Bally+Kirk+, 2005)= (MH) = (SMM) Write:<<[WBK2005] SMM NN>>
<<[WBK2005] SMM JHHMMSS+DDMMm>>
<<[WBK2005] MH NN>> N: 24+12 Object:(smm) (SIMBAD class: smmRad = Sub-Millimetric Source) Stat:is completely incorporated in Simbad Note:Optical, NIR and SCUBA SMM data of the region surrounding Barnard 1.
N=12 smm sources, and N=24 'MH' shocks that are visible in H2 but have no optical counterpart (HH number cannot be assigned). in source:Barnard 1 Ref:=2005AJ....130.1795W byWALAWENDER J. , BALLY J., KIRK H., JOHNSTONE D. Astron. J., 130, 1795-1804 (2005) Multiple outflows and protostars in Barnard 1. oTable 1: <[WBK2005] SMM NN> (Nos 1-12) = <[WBK2005] SMM JHHMMSS+DDMMm> N=12. Table 3: <[WBK2005] MH NN> (Nos 1-12). Ref:=2009AJ....137.3254W byWALAWENDER J. , REIPURTH B., BALLY J. Astron. J., 137, 3254-3262 (2009) Multiple outflows and protostars in Barnard 1. II. Deep optical and near-infrared images. oTable 1: <[WBK2005] MH NN> (Nos 13-24) added. Originof the Acronym: S = Created by Simbad, the CDS Database
© Université de Strasbourg/CNRS
• Contact