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Table · dataset · 2013

Far-UV spectroscopy of T Tau stars

Listed in IVOA Registry (Virtual Observatory)

We present a far-ultraviolet (FUV) spectral atlas consisting of spectra of 91 pre-main-sequence stars.

Description

Most stars in this sample were observed with the Space Telescope Imaging Spectrograph and Advanced Camera for Surveys on the Hubble Space Telescope (HST). A few archival spectra from the International Ultraviolet Explorer and the Goddard High Resolution Spectrograph on HST are included for completeness.

We find strong correlations among the OI{lambda}1304 triplet, the SiIV {lambda}{lambda}1394/1403 doublet, the CIV{lambda}1549 doublet, and the HeII {lambda}1640 line luminosities. For classical T Tauri stars (CTTSs), we also find strong correlations between these lines and the accretion luminosity, suggesting that these lines form in processes related to accretion. These FUV line fluxes and X-ray luminosity correlate loosely with large scatters.

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The FUV emission also correlates well with H{alpha}, H{beta}, and CaII K line luminosities. These correlations between FUV and optical diagnostics can be used to obtain rough estimates of FUV line fluxes from optical observations. Molecular hydrogen (H_2_) emission is generally present in the spectra of actively accreting CTTSs but not the weak-lined T Tauri stars that are not accreting.

The presence of H_2_ emission in the spectrum of HD 98800N suggests that the disk should be classified as actively accreting rather than a debris disk.

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Catalogue records · 2

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Stated by source
Optical · Uv · X-Ray
Inferred from text
Astronomical sciences 72% · Imaging 75%
Provenance · 1 source records, 12 field assertions
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IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/apj/744/12114 d agoJSON v1
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