Table 2
Parameters of the CTTSs observed by CoRoT and/or FLAMES/VLT.
| Mon IDa | 2Mass IDb | SpTc | EW Hα d | ErEW d | W10%Hα d | EW Hα e | FUR06f | α IRAC g | LC h | P h | LC h | P h | Q i |
|
|
(kms-1) |
|
(2008) | (days) | (2011) | (days) | ||||||
|
|
|||||||||||||
| CSIMon-000007 | 06415304+0958028 | K7 | c | –1.47 | 3 (A) | 3 (A) | 0.75 | ||||||
| CSIMon-000011 | 06411725+0954323 | K7 | 58.3 | 3 (A) | 3 (A) | ||||||||
| CSIMon-000017 | 06413199+1000244 | K5 | 13.1 | –2.69 | 1 | 4.78 | 1 | 4.73 | -0.03 | ||||
| CSIMon-000021 | 06405944+0959454 | K5 | 7.4 | c | 2 | 3.23 | 2 | 3.16 | 0.15 | ||||
| CSIMon-000056 | 06415315+0950474 | K5 | 1.8 | w | –1.36 | 2 | 5.71 | 2 | 5.86 | 0.14 | |||
| CSIMon-000058 | 06420870+0941212 | K4.5 | 94.0 | c | – | 1 | 2.14 | 0.22 | |||||
| CSIMon-000063 | 06411193+0959412 | M2.5 | 19.4 | –1.37 | – | 3 | |||||||
| CSIMon-000090 | 06410896+0933460 | M3 | 51.0 | c | –0.88 | 3 | 3 | ||||||
| CSIMon-000103 | 06405954+0935109 | K6 | 15.6 | 0.9 | 401 | 6.4 | c | –1.14 | 1 | 1.67 | 1 | 3.35 | 0.21 |
| CSIMon-000117 | 06405413+0948434 | M2.5 | 353.0 | –2.34 | – | 3 (A) | 0.72 | ||||||
| CSIMon-000119 | 06412100+0933361 | K6 | 10.5 | 0.9 | 466 | 10.6 | c | –1.44 | 3 | 3 | 0.62 | ||
Notes. Only a portion of this table is shown here. A full version is available at the CDS. This table is ordered according to the Mon ID.
“CSIMon” is an internal identification of the CSI 2264 campaign. Elsewhere in the text “CSI” was omitted for brevity.
Spectral type obtained by Venuti et al. (2014), Dahm & Simon (2005), Rebull et al. (2002), Walker (1956).
Hα parameters obtained in this work using FLAMES spectra. We used the convention that positive Hα equivalent width indicates Hα in emission, and negative values indicate Hα in absorption. The uncertainties were obtained assuming a Poisson distribution.
Hα equivalent width obtained by Dahm & Simon (2005).
Classification as CTTS (c) and WTTS (w) by Fűrész et al. (2006).
αIRAC is the slope of the spectral energy distribution between 3.6 μm and 8 μm obtained by Teixeira et al. (2012).
CoRoT light curve morphology and photometric period obtained in this work: “1” = spot-like, “2” = AA Tau-like, “3” = non-periodic light curves. Accretion bursts and aperiodic extinction light curves are identified by (A) and (E), respectively. “UNC” = unclassified light curve and “B” = Binary.
Parameter defined by Cody et al. (2014) to distinguish periodic from aperiodic light curves. According to Cody et al. (2014), when Q> 0.6 the star is not periodic photometrically.
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