Other
Scientific paper
Dec 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...189.4901m&link_type=abstract
American Astronomical Society, 189th AAS Meeting, #49.01; Bulletin of the American Astronomical Society, Vol. 28, p.1337
Other
Scientific paper
An 8.4 GHz VLA survey of 91 recently discovered T Tauri stars from the ROSAT All-Sky Survey and pointed observations is presented. These objects lie in the vicinity of the Taurus-Auriga star-forming region (d =~ 140 pc), however some are dispersed nearly 30(deg) from known active star-forming cloud cores. This sample represents a spatially-complete, flux-limited population of X-ray bright T Tauri stars both within and away from the primary Tau-Aur stellar nurseries. Of the 91 sources, 17-29 are detected in this radio survey with a sensitivity limit of ~ 0.15 mJy. Hence 19-32% of widely distributed T Tauri stars with LX >= 5x10(28) ergs s(-1) have radio luminosity densities in excess of 3.5x10(15) erg s(-1) Hz(-1) . This detection rate and range of radio and X-ray luminosities are consistent with known young weak-lined T Tauri stars (ages ~ 10(6) ) yr) which reside within the Taurus molecular clouds, but is considerably higher than a ZAMS population such as the Pleiades (age =~ 7x10(7) yr). These T Tauri stars fit well among other active young stars on the empirical LR vs. LX diagram, implying that solar type gyrosynchrotron activity is the radio emission mechanism.
Carkner Lee
Feigelson Eric
Krautter Joachim
Mamajek Eric E.
Neuhäuser Ralph
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