Detection of Accreting, Circumstellar Gas in a λ Bootis Star: 131 Tauri-Reference-Cited by-同舟云学术

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Detection of Accreting, Circumstellar Gas in a λ Bootis Star: 131 Tauri

Published:1996-06-20 Issue:2 Volume:464 Page:L183-L186
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:

Author:

Grady C. A.,McCollum B.,Rawley L. A.,England M. N.,Groebner A.,Schlegel M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference26 articles.

1. Rotation and shell spectra among A-type dwarfs.

2. 131 Tau: another Formula Bootis star with a shell

3. Newly identified main-sequence A stars with circumstellar dust

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1. Exocomets: A spectroscopic survey;Astronomy & Astrophysics;2020-07

2. The pulsation properties of λ bootis stars I. the southern TESS sample;Monthly Notices of the Royal Astronomical Society;2020-05-08

3. IR excesses around nearby Lambda Boo stars are caused by debris discs rather than ISM bow waves;Monthly Notices of the Royal Astronomical Society;2015-12-16

4. Spectra of binaries classified asλBootis stars;Astronomy & Astrophysics;2001-09

5. A speckle interferometry survey ofλBootis stars;Astronomy & Astrophysics;2001-05

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