Details on Acronym: B
B (Blue) ***** Avoid the usage of B, prefer [TB95] Originof the Acronym: L = Found in the literature
Details on Acronym: [TB95]
[TB95] (Tafalla+Bachiller, 1995)= (B) Write:<<[TB95] BNa>>
<<[TB95] RN>> N: 3+3+15 Object:Clump (SIMBAD class: Unknown = Object of Unknown Nature) Note:In the format B stands for the Blue lobe, R for the Red lobe. The SiO condensations are aligned with IRAS 20386+6751.
See also [GHL2013] and [BDC2016]. in source:LDN 1157 Ref:=1995ApJ...443L..37T byTAFALLA M. , BACHILLER R. Astrophys. J., 443, 37-40 (1995) Ammonia emission from bow shocks in the L1157 outflow. oIRAS 3282 = IRAS 03282+3035 o<[TB95] BN> (Nos B1-B2) Ref:=2000AJ....119.1345Z byZHANG Q. , HO P.T.P., WRIGHT M.C.H. Astron. J., 119, 1345-1351 (2000) The SiO and CS emission in the molecular outflow toward L1157. oFig.3: <[TB95] BN> (No. B0) added, <[TB95] RN> (Nos R0, R1, R2). Ref:=2007MNRAS.381.1127B byBENEDETTINI M. , VITI S., CODELLA C., BACHILLER R., GUETH F., BELTRAN M.T., DUTREY A., GUILLOTEAU S. Mon. Not. R. Astron. Soc., 381, 1127-1136 (2007) The clumpy structure of the chemically active L1157 outflow. oFigs 1, 2, Table 2: <[TB95] BNa> (Nos B0a-B0e, B1a-B1d, B2a-B2c). Ref:=2009A&A...507L..25C byCODELLA C. , BENEDETTINI M., BELTRAN M.T., GUETH F., VITI S., BACHILLER R., TAFALLA M., CABRIT S., FUENTE A., LEFLOCH B. Astron. Astrophys., 507L, 25-28 (2009) Methyl cyanide as tracer of bow shocks in L1157-B1. oFig. 1, Table 1: <[TB95] BNa> (Nos B0f, B1e-B1f) added. Originof the Acronym: S = Created by Simbad, the CDS Database
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