Details on Acronym: [MBB87] | |
[MBB87] | (Mundt+Brugel+Buhrke, 1987) |
Write: | <<[MBB87] HH 34 IRS>> <<[MBB87] Haro 6-5B A>> <<[MBB87] Haro 6-5B RN>> <<[MBB87] DG Tau B A>> <<[MBB87] DG Tau B AN>> <<[MBB87] HL Tau VLA N>> <<[MBB87] HH 33-40 A>> |
N: | 1+6+2+6+2+1+2 |
Object: | Knot (SIMBAD class: Unknown = Object of Unknown Nature) |
Stat: | is completely incorporated in Simbad |
Note: | In HH 34: N=1 IRS source, 'HH 34 IRS' In Haro 6-5B field ('[BMD85] FS Tau B' in SIMBAD): N=6 knots (Nos A-F), eq. to '[EM98] FS Tau B Knot A' (Nos A-F). N=2 Reflexion Nebula (Nos R1-R2), eq. to '[EM98] FS Tau B R1 and R2' In DG Tau B field ('[MF83] DG Tau B' in SIMBAD): N=6+2 knots (Nos A-C, F-H, A1-A2), eq. to '[EM98] DG Tau B Knot AN' In HL Tau: N=1 VLA radio-source In HH 33-40 ('NAME HH 33-40' in SIMBAD): N=2 knots (Nos A-B) |
Ref: | =1987ApJ...319..275M |
by | MUNDT R. , BRUGEL E.W., BUHRKE T. |
Astrophys. J., 319, 275-303 (1987) | |
Jets from young stars : CCD imaging, long-slit spectroscopy and interpretation of existing data. | |
o | Fig.2, Table 2: <[MBB87] HH 34 IRS> N=1. Fig.5: <[MBB87] Haro 6-5B A> (Nos A-B), <[MBB87] Haro 6-5B RN> (Nos R1-R2). Fig.7: <[MBB87] DG Tau B A> (Nos A-C). Fig.13, Table 3: <[MBB87] HL Tau VLA 1> N=1. Fig.14: <[MBB87] HH 33-40 A> (Nos A-B). |
Ref: | =1991A&A...252..740M |
by | MUNDT R. , RAY T.P., RAGA A.C. |
Astron. Astrophys., 252, 740-761 (1991) | |
Collimation of stellar objects - constraints from the observed spatial structure. II. Observational results. | |
o | Fig.8: <[MBB87] Haro 6-5B A> (Nos C-F) added. Fig.12: <[MBB87] DG Tau B AN> (Nos A1-A2, F-H) added. |
Origin | of the Acronym: S = Created by Simbad, the CDS Database |