VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/AJ/105/226
  UMa Group (Soderblom+ 1993)
Post annotation
  
1.J/AJ/105/226/table5Spectroscopic membership indicators for UMaG solar-type stars (46 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)
  Member (char) [abc] a: Probable spectroscopic member b: Possible spectroscopic member c: Probable spectroscopic non-member (meta.code.member)
  Wooley (char) Number in catalog of Woolley, et al. (1970) (meta.id)
  HD/HDE  Henry Draper number (meta.id;meta.main)
  m_HD/HDE (char) Multiplicity index on HD or HDE number (meta.code.multip)
  HR   []? Harvard Revised (Bright Star) number (meta.id)
  m_HR (char) Multiplicity index on HR number (meta.code.multip)
  Name (char) Other name (meta.id)
  Sp (char) Spectral type (Note 1)   (src.spType)
  B-V mag []? (B-V) color from Nicolet (1978) or Woolley et al. (1970) (phot.color;em.opt.B;em.opt.V)
  u_B-V (char) uncertainty flag on B-V (meta.code.error)

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 (i)indexed column
  Teff K []? Effective temperature (phys.temperature.effective)
  u_Teff (char) uncertainty flag on Teff (meta.code.error)
  l_R' (char) [<H] limit flag on R'(HK). An 'H' indicating that Log(R') is instead an eye estimate of H and K emission strength from Wilson & Woolley (1970) (meta.code.error)
  logR'   []? Chromospheric flux ratio of the Ca II H and K emission features (phot.flux;arith.ratio)
  u_logR' (char) uncertainty flag on R' (meta.code.error)
  n_R(hk) (char) [I] An 'I', indicating logR(hk) is an I(Mg II) value (meta.note)
  logR(hk)   []? Rescaled index, the Mg II h and k emission flux divided by the stellar bolometric flux and reduced to the scale of the Ca II H and K emission in logR' (phot.flux;arith.ratio)
  l_R(TR) (char) limit flag on R(TR) (meta.code.error)
  logR(TR)   []? Rescaled index, the emission flux of three strong features in IUE spectra (N I 1240 A, Si IV 1400 A, and C IV 1550 A) combined to produce an index of emission from the star's transition region (TR), reduced to the scale of the Ca II H and K lines as a (spect.index)
  l_R(Halpha) (char) uncertainty flag on R(Halpha) (meta.code.error)
  logR(Halpha)   []? Rescaled index, logR(Halpha). (spect.index)
  u_R(Halpha) (char) rms uncertainty on R(Halpha) (meta.code.error)
  l_R(IRT) (char) uncertainty flag on R(IRT) (meta.code.error)
  logR(IRT)   []? Rescaled index, for the Ca II infrared triplet. (spect.index)
  l_vsini (char) limit flag on vsini (meta.code.error)
  vsini km/s []? Rotational velocity (phys.veloc.rotat)
  e_vsini km/s []? rms uncertainty in v sin i (stat.error)

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