Details on Acronym: B | |
B | (Blue) |
***** | Avoid the usage of B, prefer [TB95] |
Origin | of 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 |
by | TAFALLA M. , BACHILLER R. |
Astrophys. J., 443, 37-40 (1995) | |
Ammonia emission from bow shocks in the L1157 outflow. | |
o | IRAS 3282 = IRAS 03282+3035 |
o | <[TB95] BN> (Nos B1-B2) |
Ref: | =2000AJ....119.1345Z |
by | ZHANG 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. | |
o | Fig.3: <[TB95] BN> (No. B0) added, <[TB95] RN> (Nos R0, R1, R2). |
Ref: | =2007MNRAS.381.1127B |
by | BENEDETTINI 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. | |
o | Figs 1, 2, Table 2: <[TB95] BNa> (Nos B0a-B0e, B1a-B1d, B2a-B2c). |
Ref: | =2009A&A...507L..25C |
by | CODELLA 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. | |
o | Fig. 1, Table 1: <[TB95] BNa> (Nos B0f, B1e-B1f) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |