VizieR

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

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/MNRAS/465/3039
  Eruptive variable protostars from VVV EW (Contreras+, 2017)
ReadMe+ftp
2017MNRAS.465.3039C
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/465/3039/table1(c)Characteristics of the spectroscopic sample of VVV high-amplitude variables (37 rows)
2.J/MNRAS/465/3039/table3(c)Equivalent widths of common features found in near-IR spectra of YSOs detected in our VVV sample (40 rows)
3.J/MNRAS/465/3039/table4Radial velocities (17 rows)
4.J/MNRAS/465/3039/table5Accretion luminosity from luminosity of the Brγ line (23 rows)
5.J/MNRAS/465/3039/tabled1Parameters derived from the Robitaille et al. (2007ApJS..169..328R) models SED fitting as explained in the text (37 rows)

Simple ConstraintList Of Constraints
 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (1)No  Sequential number (meta.record)
   (ALL)VName (char) Variable name (VVVvNNN, [CLM2017] VVVvNNN in Simbad) (meta.id;meta.main)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)Jmag mag (n) J magnitude (phot.mag;em.IR.J)
  (1)e_Jmag mag (n) rms uncertainty on Jmag (stat.error;phot.mag;em.IR.J)
  (1)Hmag mag (n) H magnitude (phot.mag;em.IR.H)
  (1)e_Hmag mag (n) rms uncertainty on Hmag (stat.error;phot.mag;em.IR.H)
  (1)Ksmag mag (n) Ks magnitude (phot.mag;em.IR.K)
  (1)e_Ksmag mag (n) rms uncertainty on Ksmag (stat.error;phot.mag;em.IR.K)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)DKsmag mag Ksmax-Ksmin difference (phot.mag;arith.diff)
  (1)alpha  (n) Slope of the SED, from Paper I (spect.index)
  (1)dSFR kpc (n) likely distance to our objects estimated from SIMBAD (pos.distance)
  (1)Shape (char) Shape, from Paper I (src.morph.type)
  (1+2+4+5)Type (char) Type, this paper (Note 1)   (src.morph.type)
  (2)more (char) indicates data in other tables (meta.ref.url)
  (2)n_VName (char) Observation number (meta.note)
  (2)EWH2 0.1nm (n) H2 (2.12um) equivalent width (Note 1)   (spect.line.eqWidth)
  (2)e_EWH2 0.1nm (n) rms uncertainty on EWH2 (stat.error)
  (2)EWBrg 0.1nm (n) Brγ (2.16um) equivalent width (Note 1)   (spect.line.eqWidth)
  (2)e_EWBrg 0.1nm (n) rms uncertainty on EWBrg (stat.error)
  (2)EWNaI 0.1nm (n) NaI (2.21um) equivalent width (Note 1)   (spect.line.eqWidth)
  (2)e_EWNaI 0.1nm (n) rms uncertainty on EWNaI (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)EWCaI 0.1nm (n) CaI (2.26um) equivalent width (Note 1)   (spect.line.eqWidth)
  (2)e_EWCaI 0.1nm (n) rms uncertainty on EWCaI (stat.error)
  (2)EW12CO 0.1nm (n) 12CO (2.293um) equivalent width (1) (Note 2)   (spect.line.eqWidth;em.line.CO)
  (2)e_EW12CO 0.1nm (n) rms uncertainty on EW12CO (stat.error)
  (2)EWMgI 0.1nm (n) MgI (2.28um) equivalent width (Note 1)   (spect.line.eqWidth)
  (2)e_EWMgI 0.1nm (n) rms uncertainty on EWMgI (stat.error)
  (2)PapI (char) Display the Contreras Pena et al. (2017, Cat. J/MNRAS/465/3011) data (meta.ref.url)
  (2)_RA deg (i) Positions from vVVV catalog (right ascension part) (pos.eq.ra;meta.main)
  (2)_DE deg (i) Positions from vVVV catalog (declination part) (pos.eq.dec;meta.main)
  (3)Vlsr km/s LSR velocity (phys.veloc;pos.lsr)
  (3)e_Vlsr km/s rms uncertainty on Vlsr (stat.error;phys.veloc;pos.lsr)
  (3)dnear kpc (n) Near distance (pos.distance)
  (3)dfar kpc Far distance (pos.distance)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)State (char) Approximate state (from the LC) at which the spectrum was taken (meta.note)
  (4)AKs mag Absorption in Ks band (phys.absorption)
  (4)n_AKs (char) Note on AKs (Note 1)   (meta.note)
  (4+5)Dist kpc Distance (pos.distance)
  (4)n_Dist (char) Note on Distance (Note 1)   (meta.note)
  (4)Lacc1 Lsun Accretion luminosity from Calvet et al. (2004AJ....128.1294C) (phys.luminosity)
  (4)Lacc2 Lsun Accretion luminosity from Muzerolle et al. (1998AJ....116.2965M) (phys.luminosity)
  (5)M* Msun Stellar mass (phys.mass)
  (5)E_M* Msun Error on M* (upper value) (stat.error;stat.max)
  (5)e_M* Msun Error on M* (lower value) (stat.error)
  (5)logdMenv/dt [Msun/yr](n) Envelope infall rate (phys.mass.loss)
  (5)e_logdMenv/dt [Msun/yr](n) rms uncertainty on logdMenv/dt (stat.error)
  (5)logdMdisc/dt [Msun/yr]Disc mass accretion rate (arith.rate;phys.mass)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)e_logdMdisc/dt [Msun/yr]rms uncertainty on logdMdisc/dt (stat.error)
  (5)logAge [yr] Age (time.age)
  (5)e_logAge [yr] rms uncertainty on Age (stat.error;time.age)
  (5)E_Dist kpc Error on Dist (upper value) (stat.error;stat.max)
  (5)e_Dist kpc Error on Dist (lower value) (stat.error)
  (5)logLbol [Lsun] Bolometric luminosity of the system (phys.luminosity)
  (5)e_logLbol [Lsun] rms uncertainty on logLbol (stat.error)
  (5)chi2/N  chi2 per data point of the best-fitting model (stat.fit.chi2)
  (5)Nfits  Number of fits used to derive the weighted mean values (meta.number)
  (5)Nfits2  Number of models which envelope infall rate could be derived (meta.number)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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