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  Be stars near-IR excess (Dougherty+, 1994)
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1.J/A+A/290/609/table1Excess colours of 144 Be stars (144 rows)

Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  HR   []? HR number (
  HD  HD number (;meta.main)
  Source (char) Source name (
  Sp (char) Spectral type (from the Bright Star Catalogue) (src.spType)
  E[B-V]1 mag Excess [B-V] colour (calculated from spectral type) (phot.color.excess)
  E[B-V]2 mag []? Excess [B-V] colour from the 2175 angstrom interstellar absorption feature (Beeckmans and Hubert-Delplace (1980)) and converted using E(B-V) = 0.84E[B-V] (Cramer, 1984) (phot.color.excess)
  E[V-J] mag Excess [V-J] colour (phot.color.excess)
  E[V-H] mag []? Excess [V-H] colour (phot.color.excess)
  E[V-K] mag []? Excess [V-K] colour (phot.color.excess)
  E[V-L] mag []? excess [V-L] colour (phot.color.excess)
  Ref (char) Comment for the source of the observations: a) Dougherty et al., 1991 b) Dachs et al., 1988 c) Burki et al., in preparation Visual observations from Burki et al. (in preparation) except when n_Ref. = 5 (meta.note)
  n_Ref (char) If n_Ref = 5, the visual observations are taken from the catalogue of Rufener (1988) (meta.note)

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