Dictionary of Nomenclature of Celestial Objects

 Y. (MB)
Details on Acronym:   [MBB87]
  
[MBB87]
 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
     byMUNDT 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.
oFig.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
     byMUNDT 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.
oFig.8: <[MBB87] Haro 6-5B A> (Nos C-F) added. Fig.12: <[MBB87] DG Tau    B AN> (Nos A1-A2, F-H) added.
 Originof the Acronym: S = Created by Simbad, the CDS Database