| dc.contributor.author | Hellier, C | |
| dc.contributor.author | Naylor, T | |
| dc.date.accessioned | 2017-02-13T15:06:16Z | |
| dc.date.issued | 1998-04-01 | |
| dc.description.abstract | Using the latest compilation of cataclysmic variable orbital periods by Ritter & Kolb we argue against Verbunt's conclusion that the period gap is not significant for nova-like variables. We also discuss the relation of the VY Scl stars to the dwarf novae. | en_GB |
| dc.identifier.citation | Vol. 295, No. 2, pp. L50-L52. | en_GB |
| dc.identifier.doi | 10.1046/j.1365-8711.1998.01556.x | |
| dc.identifier.uri | http://hdl.handle.net/10871/25799 | |
| dc.language.iso | en | en_GB |
| dc.publisher | Oxford University Press | en_GB |
| dc.relation.url | http://dx.doi.org/10.1046/j.1365-8711.1998.01556.x | en_GB |
| dc.relation.url | http://arxiv.org/abs/astro-ph/9802041v1 | en_GB |
| dc.rights | This is the author accepted manuscript. The final version is available from Oxford University Press via the DOI in this record. | en_GB |
| dc.subject | astro-ph | en_GB |
| dc.subject | astro-ph | en_GB |
| dc.subject | accretion | en_GB |
| dc.subject | accretion disks | en_GB |
| dc.subject | binaries: close | en_GB |
| dc.subject | novae | en_GB |
| dc.subject | cataclysmic variables | en_GB |
| dc.title | On the orbital period distribution of cataclysmic variables | en_GB |
| dc.type | Article | en_GB |
| dc.date.available | 2017-02-13T15:06:16Z | |
| dc.identifier.issn | 0035-8711 | |
| dc.description | 3 pages, 3 figures, LaTeX, To appear in MNRAS. Also at http://www.astro.keele.ac.uk/~ch/ | en_GB |
| dc.identifier.eissn | 1365-2966 | |
| dc.identifier.journal | Monthly Notices of the Royal Astronomical Society | en_GB |
