Two families of comets falling onto Beta PIctoris
dc.contributor.author | Pollard KR | |
dc.contributor.author | Barnes SI | |
dc.contributor.author | Persson SI | |
dc.contributor.author | Tobin W | |
dc.date.accessioned | 2018-06-26T02:16:05Z | |
dc.date.available | 2018-06-26T02:16:05Z | |
dc.date.issued | 2017 | en |
dc.date.updated | 2018-02-27T01:47:38Z | |
dc.description.abstract | The 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.uri | http://hdl.handle.net/10092/15602 | |
dc.language.iso | en | |
dc.subject.anzsrc | Fields of Research::51 - Physical sciences::5101 - Astronomical sciences::510109 - Stellar astronomy and planetary systems | en |
dc.title | Two families of comets falling onto Beta PIctoris | en |
dc.title.alternative | Two families of comets falling onto B Pictoris | en |
dc.type | Conference Contributions - Other | en |
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