Explanation of the abbreviations used

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Col 9. IRAS Source

  • N: No IRAS source.
  • Y: Iras source.
  • ?: IRAS detection hole, see Weintraub 1990.
  • O: Offset between optical- and IRAS-source, see sect. 3.3. and Table 2.

    • Col. 11. Remarks

  • Bin: Binary
  • Em: Emission
  • Neb: Nebula
  • Poss: Possible
  • Symb: Symbiotic star
  • Cand: Candidate
  • HHO: Herbig-Haro object
  • NIRE: Near Infrared Excess
  • Ref Neb: Reflection Nebula
  • Var: Variable
  • Class Be: Classical Be-star
  • HP(I): High (Intrinsic) Pol, 1-3 %
  • N PN: No Planetary Nebula
  • Reg: Region
  • VHP(I): Very High (Intrinsic) Pol, > 3%
  • Comp: Companion
  • L*: Stellar luminosity
  • Obs Reg: Obscured Region
  • Rej: Rejected
  • DST: Double star
  • LBV: Luminous Blue Variable
  • PN: Planetary Nebula
  • Sc: Source
  • Ecl Bin: Eclipsing Binary
  • LP(I): Low (Intrinsic) Pol, < 1%
  • Pol: Polarization
  • Sp T: Spectral Type
    • [Table I | Table II | Table III | Table IVa | Table IVb | Table V | Table VI | Remarks | Abbreviations | References | Index]
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    mvandena@eso.org Last modified: 09/03/2002 16:43:32 undefined, undefined