uυby Hβ photometry of UV-bright stars
uυby Hβ photometry is presented for 90 stars taken from an early version of the Carnochan & Wilson catalogue of stars that have very negative UV colours. Two have definite UV excesses, (HD 36629, and HD 81307). Four early-B stars have UV colours too positive for their visible classification, and...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 1985-01, Vol.212 (1), p.77-91 |
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creator | Wade, Brian R. Smith, Lindsey F. |
description | uυby Hβ photometry is presented for 90 stars taken from an early version of the Carnochan & Wilson catalogue of stars that have very negative UV colours. Two have definite UV excesses, (HD 36629, and HD 81307). Four early-B stars have UV colours too positive for their visible classification, and β-indices that indicate higher luminosities than appear possible on galactic distribution grounds. Six late-B stars appear to have discordant flux distributions for which there are no obvious explanations. We suggest that the high population of subluminous stars derived by Carnochan & Wilson is the product of the statistical treatment used and the extreme patchiness in the interstellar absorption which gives rise to large numbers of little-reddened stars. |
doi_str_mv | 10.1093/mnras/212.1.77 |
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We suggest that the high population of subluminous stars derived by Carnochan & Wilson is the product of the statistical treatment used and the extreme patchiness in the interstellar absorption which gives rise to large numbers of little-reddened stars.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1093/mnras/212.1.77</identifier><language>eng</language><publisher>Oxford, UK: Oxford University Press</publisher><ispartof>Monthly notices of the Royal Astronomical Society, 1985-01, Vol.212 (1), p.77-91</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Wade, Brian R.</creatorcontrib><creatorcontrib>Smith, Lindsey F.</creatorcontrib><title>uυby Hβ photometry of UV-bright stars</title><title>Monthly notices of the Royal Astronomical Society</title><description>uυby Hβ photometry is presented for 90 stars taken from an early version of the Carnochan & Wilson catalogue of stars that have very negative UV colours. Two have definite UV excesses, (HD 36629, and HD 81307). Four early-B stars have UV colours too positive for their visible classification, and β-indices that indicate higher luminosities than appear possible on galactic distribution grounds. Six late-B stars appear to have discordant flux distributions for which there are no obvious explanations. We suggest that the high population of subluminous stars derived by Carnochan & Wilson is the product of the statistical treatment used and the extreme patchiness in the interstellar absorption which gives rise to large numbers of little-reddened stars.</description><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1985</creationdate><recordtype>article</recordtype><recordid>eNpjYBAzNNAzNLA01s_NK0os1jcyNNIz1DM3Z2LgNDQ2M9U1sjQzY2HgNDAwNtW1MDc05GDgKi7OMjAwMDE2MuNkUC8935pUqeBxbpNCQUZ-SX5uaklRpUJ-mkJomG5SUWZ6RolCcUliUTEPA2taYk5xKi-U5mbQdXMNcfbQzSwuSa2ILyjKzE0sqoxPLMqONzM3NjeN94iIijeyCDR3d_ExiA82JlU9AFvOPhg</recordid><startdate>19850101</startdate><enddate>19850101</enddate><creator>Wade, Brian R.</creator><creator>Smith, Lindsey F.</creator><general>Oxford University Press</general><scope>BSCLL</scope></search><sort><creationdate>19850101</creationdate><title>uυby Hβ photometry of UV-bright stars</title><author>Wade, Brian R. ; Smith, Lindsey F.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-istex_primary_ark_67375_HXZ_28Q7GDL0_S3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1985</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Wade, Brian R.</creatorcontrib><creatorcontrib>Smith, Lindsey F.</creatorcontrib><collection>Istex</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wade, Brian R.</au><au>Smith, Lindsey F.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>uυby Hβ photometry of UV-bright stars</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><date>1985-01-01</date><risdate>1985</risdate><volume>212</volume><issue>1</issue><spage>77</spage><epage>91</epage><pages>77-91</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>uυby Hβ photometry is presented for 90 stars taken from an early version of the Carnochan & Wilson catalogue of stars that have very negative UV colours. Two have definite UV excesses, (HD 36629, and HD 81307). Four early-B stars have UV colours too positive for their visible classification, and β-indices that indicate higher luminosities than appear possible on galactic distribution grounds. Six late-B stars appear to have discordant flux distributions for which there are no obvious explanations. We suggest that the high population of subluminous stars derived by Carnochan & Wilson is the product of the statistical treatment used and the extreme patchiness in the interstellar absorption which gives rise to large numbers of little-reddened stars.</abstract><cop>Oxford, UK</cop><pub>Oxford University Press</pub><doi>10.1093/mnras/212.1.77</doi></addata></record> |
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source | Electronic Journals Library; OUP_牛津大学出版社OA刊; Oxford University Press Journals Digital Archive Legacy |
title | uυby Hβ photometry of UV-bright stars |
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