| dc.contributor.author | Vink, J.S. | |
| dc.contributor.author | Drew, J.E. | |
| dc.contributor.author | Harries, T.J. | |
| dc.contributor.author | Oudmaijer, R.D. | |
| dc.date.accessioned | 2008-02-21T10:53:21Z | |
| dc.date.available | 2008-02-21T10:53:21Z | |
| dc.date.issued | 2002 | |
| dc.identifier.citation | Vink , J S , Drew , J E , Harries , T J & Oudmaijer , R D 2002 , Are all Young Stars Disc Accretors . in In: Procs of the Hot Star Workshop III: the Earliest Stages of Massive Star Birth - ASP Conf Series Vol.267 . Astronomical Society of the Pacific , pp. 439-440 . | |
| dc.identifier.isbn | 978-1-58381-603-5 | |
| dc.identifier.isbn | 1-58381-107-9 | |
| dc.identifier.other | dspace: 2299/1670 | |
| dc.identifier.other | ORCID: /0000-0003-1192-7082/work/62750040 | |
| dc.identifier.uri | http://hdl.handle.net/2299/1670 | |
| dc.description | Original paper can be found at: http://www.astrosociety.org/pubs/cs/253.html--Copyright Astronomical Society of the Pacific | |
| dc.description.abstract | We demonstrate the importance of Ha spectro-polarimetry in constraining the geometry of Herbig Ae/Be stars. We find that discs are common in Herbig Ae and Be stars, although different polarization signatures may imply different modes of accretion. | en |
| dc.format.extent | 142718 | |
| dc.language.iso | eng | |
| dc.publisher | Astronomical Society of the Pacific | |
| dc.relation.ispartof | In: Procs of the Hot Star Workshop III: the Earliest Stages of Massive Star Birth - ASP Conf Series Vol.267 | |
| dc.title | Are all Young Stars Disc Accretors | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
