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J/MNRAS/415/103 IPHAS T Tauri candidates in IC 1396 (Barentsen+, 2011)
The following files can be converted to FITS (extension .fit or fit.gz)
table[be]1.dat tablec1.dat tabled1.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/415/103
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Beginning of ReadMe :J/MNRAS/415/103 IPHAS T Tauri candidates in IC 1396 (Barentsen+, 2011)
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T Tauri candidates and accretion rates using IPHAS:
method and application to IC 1396.
Barentsen G., Vink J.S., Drew J.E., Greimel R., Wright N.J., Drake J.J.,
Martin E.L., Valdivielso L., Corradi R.L.M.
<Mon. Not. R. Astron. Soc., 415, 103-132 (2011)>
=2011MNRAS.415..103B
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ADC_Keywords: Clusters, open ; Stars, pre-main sequence ; Photometry, infrared ;
Photometry, H-alpha ; Photometry, millimetric/submm
Keywords: accretion, accretion discs - stars: pre-main-sequence -
stars: variables: T Tauri, Herbig Ae/Be -
open clusters and associations: individual: IC 1396
Abstract:
The Isaac Newton Telescope (INT) Photometric H-Alpha Survey (IPHAS) is
a 1800deg^2^ survey of the Northern Galactic Plane, reaching down to
r' 21. We demonstrate how the survey can be used to (1) reliably
select classical T Tauri star candidates and (2) constrain the mass
accretion rates with an estimated relative uncertainty of 0.6dex.
IPHAS is a necessary addition to spectroscopic surveys because it
allows large and uniform samples of accretion rates to be obtained
with a precise handle on the selection effects.
We apply the method on a region of 7deg^2^ towards the HII region
IC 1396 in Cepheus OB2 and identify 158 pre-main-sequence candidates
with masses between 0.2 and 2.0M_sun_ and accretion rates between
10-9.2 and 10-7.0M_sun_/yr.