The Appearance and Disappearance of Exocomet Gas Absorption

CaII K-line (3933 Å) absorption profiles observed towards 15 A-type and two B-type stars with known (or suspected) debris disks, in addition to archival spectral data for three A-type stars, are presented. Inspection of the extracted CaII K-line absorption lines has determined that one late B-type (...

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Main Authors: Barry Y. Welsh, Sharon L. Montgomery
Format: Article
Language:English
Published: Wiley 2015-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2015/980323
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author Barry Y. Welsh
Sharon L. Montgomery
author_facet Barry Y. Welsh
Sharon L. Montgomery
author_sort Barry Y. Welsh
collection DOAJ
description CaII K-line (3933 Å) absorption profiles observed towards 15 A-type and two B-type stars with known (or suspected) debris disks, in addition to archival spectral data for three A-type stars, are presented. Inspection of the extracted CaII K-line absorption lines has determined that one late B-type (HD 58647) and four new A-type (HD 56537, HD 64145, HD 108767, and HD 109573) stellar systems exhibit short-term (night-to-night) absorption variation within these profiles. This variability is due to the liberation of gas from falling evaporating bodies (the so-called FEBs activity) on the grazing approach of exocomets towards their parent star. Also we present archival spectra of the FeI λ3860 Å and CaII K-lines towards β Pictoris (HD 39060) that, for the first time, reveal the absorption signatures of FEB activity at similar velocities in both line profiles. FEB-hosting stars seem to be of an earlier type (on average spectral type Al.8 as compared with A3.1) than those where no FEB activity has been observed. This could be due to stellar activity levels (such as chromospheric activity or nonradial pulsations) being of a higher level within the atmospheres of these hotter A-type stars.
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spelling doaj-art-e61315e1375f47f089c442d34f7b45a72025-02-03T05:51:23ZengWileyAdvances in Astronomy1687-79691687-79772015-01-01201510.1155/2015/980323980323The Appearance and Disappearance of Exocomet Gas AbsorptionBarry Y. Welsh0Sharon L. Montgomery1Experimental Astrophysics Group, Space Sciences Laboratory, University of California, 7 Gauss Way, Berkeley, CA 94720, USADepartment of Chemistry, Mathematics & Physics, Clarion University, Clarion, PA 16214, USACaII K-line (3933 Å) absorption profiles observed towards 15 A-type and two B-type stars with known (or suspected) debris disks, in addition to archival spectral data for three A-type stars, are presented. Inspection of the extracted CaII K-line absorption lines has determined that one late B-type (HD 58647) and four new A-type (HD 56537, HD 64145, HD 108767, and HD 109573) stellar systems exhibit short-term (night-to-night) absorption variation within these profiles. This variability is due to the liberation of gas from falling evaporating bodies (the so-called FEBs activity) on the grazing approach of exocomets towards their parent star. Also we present archival spectra of the FeI λ3860 Å and CaII K-lines towards β Pictoris (HD 39060) that, for the first time, reveal the absorption signatures of FEB activity at similar velocities in both line profiles. FEB-hosting stars seem to be of an earlier type (on average spectral type Al.8 as compared with A3.1) than those where no FEB activity has been observed. This could be due to stellar activity levels (such as chromospheric activity or nonradial pulsations) being of a higher level within the atmospheres of these hotter A-type stars.http://dx.doi.org/10.1155/2015/980323
spellingShingle Barry Y. Welsh
Sharon L. Montgomery
The Appearance and Disappearance of Exocomet Gas Absorption
Advances in Astronomy
title The Appearance and Disappearance of Exocomet Gas Absorption
title_full The Appearance and Disappearance of Exocomet Gas Absorption
title_fullStr The Appearance and Disappearance of Exocomet Gas Absorption
title_full_unstemmed The Appearance and Disappearance of Exocomet Gas Absorption
title_short The Appearance and Disappearance of Exocomet Gas Absorption
title_sort appearance and disappearance of exocomet gas absorption
url http://dx.doi.org/10.1155/2015/980323
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