Two families of comets falling onto Beta PIctoris

dc.contributor.authorPollard KR
dc.contributor.authorBarnes SI
dc.contributor.authorPersson SI
dc.contributor.authorTobin W
dc.date.accessioned2018-06-26T02:16:05Z
dc.date.available2018-06-26T02:16:05Z
dc.date.issued2017en
dc.date.updated2018-02-27T01:47:38Z
dc.description.abstractThe young A6 V star β Pictoris shows variable, velocity-shifted absorptions in the Ca II H & K lines, which are attributed to infalling, evaporating, comet-like bodies (exocomets). We have analyzed Ca II H & K absorptions in β Pictoris obtained with the 1.0- metre telescope at the University of Canterbury Mt John Observatory, New Zealand. Our data show a clear division of the exocomets into the two families identified by Kiefer et al. (2014).en
dc.identifier.urihttp://hdl.handle.net/10092/15602
dc.language.isoen
dc.subject.anzsrcFields of Research::51 - Physical sciences::5101 - Astronomical sciences::510109 - Stellar astronomy and planetary systemsen
dc.titleTwo families of comets falling onto Beta PIctorisen
dc.title.alternativeTwo families of comets falling onto B Pictorisen
dc.typeConference Contributions - Otheren
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