Details on Acronym: [BCM90] | |
[BCM90] | (Bachiller+Cernicharo+Martin-Pintado+, 2000) |
Write: | <<[BCM90] U-star>> <<[BCM90] B>> <<[BCM90] BN>> <<[BCM90] R>> <<[BCM90] RN>> <<[BCM90] BW>> <<[BCM90] RW>> |
N: | 1+2+8+2 |
Object: | Feature (SIMBAD class: Unknown = Object of Unknown Nature) |
Note: | p.178: N=1 'U-star', the letter 'U' stands for 'Unseen', Hypothetical exciting star of the outflow. In the outflow, the gaz is concentrated in 2 lobes, blueshifted lobe 'B' and redshifted lobe 'R'. Redshifted emission is divided into 2 features 'RN' and 'RS'. Bullets (Nos B1-B4) have their counterparts (Nos R1-R4) at symmetric positions with respect to the U-star. |
in source: | LDN 1448 |
Ref: | =1990A&A...231..174B |
by | BACHILLER R. , CERNICHARO J., MARTIN-PINTADO J., TAFALLA M., LAZAREFF B. |
Astron. Astrophys., 231, 174-186 (1990) | |
High-velocity molecular bullets in a fast bipolar outflow near L 1448/IRS 3. | |
o | L 1448/IRS 3 = [BC86b] LDN 1448 IRS 3. |
o | Text, p.178: <[BCM90] U-star> N=1. Figs 8, 9: <[BCM90] A> (Nos R, B), <[BCM90] AW> (Nos RN, RS), <[BCM90] AN> (Nos R1-R4, B1-B4). |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |