EMISSION LINES IN THE SPECTRA OF THE RV TAURI STARS U MONOCEROTIS AND AC HERCULIS
Strong metallic emission lines have been observed in the spectra of the RV Tauri stars U Mon and AC Her near recent light minima. While these two variables differ in a number of significant respects, the metallic emission spectra are quite similar, resembling the emission that we have previously rep...
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| Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1984-06, Vol.96 (580), p.432-436 |
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| container_title | Publications of the Astronomical Society of the Pacific |
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| creator | BOPP, BERNARD W. |
| description | Strong metallic emission lines have been observed in the spectra of the RV Tauri stars U Mon and AC Her near recent light minima. While these two variables differ in a number of significant respects, the metallic emission spectra are quite similar, resembling the emission that we have previously reported as present in the spectrum of R Sct at a deep minimum. The data appear to support Baird's shock-wave model for the spectral behavior of RV Tauri stars. |
| doi_str_mv | 10.1086/131359 |
| format | Article |
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While these two variables differ in a number of significant respects, the metallic emission spectra are quite similar, resembling the emission that we have previously reported as present in the spectrum of R Sct at a deep minimum. The data appear to support Baird's shock-wave model for the spectral behavior of RV Tauri stars.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/131359</identifier><language>eng</language><publisher>Legacy CDMS: The Astronomical Society of the Pacific</publisher><subject>Absorption spectra ; Astrophysics ; Emission spectra ; Light curves ; Line spectra ; Radial velocity ; RV Tauri variables ; Spectroscopy ; Stellar spectra ; Visible spectrum ; Wavelengths</subject><ispartof>Publications of the Astronomical Society of the Pacific, 1984-06, Vol.96 (580), p.432-436</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c259t-7586bafd12230ad0cebe913c01252689dc97b8bb44052dcc2dee23b6bf6bd2173</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/40678342$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/40678342$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,780,784,803,27924,27925,58017,58250</link.rule.ids></links><search><creatorcontrib>BOPP, BERNARD W.</creatorcontrib><title>EMISSION LINES IN THE SPECTRA OF THE RV TAURI STARS U MONOCEROTIS AND AC HERCULIS</title><title>Publications of the Astronomical Society of the Pacific</title><description>Strong metallic emission lines have been observed in the spectra of the RV Tauri stars U Mon and AC Her near recent light minima. While these two variables differ in a number of significant respects, the metallic emission spectra are quite similar, resembling the emission that we have previously reported as present in the spectrum of R Sct at a deep minimum. The data appear to support Baird's shock-wave model for the spectral behavior of RV Tauri stars.</description><subject>Absorption spectra</subject><subject>Astrophysics</subject><subject>Emission spectra</subject><subject>Light curves</subject><subject>Line spectra</subject><subject>Radial velocity</subject><subject>RV Tauri variables</subject><subject>Spectroscopy</subject><subject>Stellar spectra</subject><subject>Visible spectrum</subject><subject>Wavelengths</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1984</creationdate><recordtype>article</recordtype><sourceid>CYI</sourceid><recordid>eNpFkMFPgzAchRujiXPqX6BJT97QX1ug5UiQuSYMlIJXQqEkW7YxKTv43-vE6Onl5X35Dg-hWwKPBIT_RBhhXnCGZsRjwmGCs3M0AwDX8amAS3Rl7QaAEEFght7ilVRKZilOZBorLFNcLGOsXuOoyEOcLX5q_o6LsMwlVkWYK1ziVZZmUZxnhVQ4TJ9xGOFlnEdlItU1uujqrTU3vzlH5SIuoqWTZC8yChOnoV4wOtwTvq67llDKoG6hMdoEhDVAqEd9EbRNwLXQ2nXBo23T0NYYyrSvO1-3lHA2Rw-T9zD0H0djx2q3to3Zbuu96Y-2oi7lnAnyDzZDb-1guuowrHf18FkRqE6PVdNj3-DdBO5rW1f7cbAVCYQL4HHOT577ad7YsR_-JC74XDCXsi9JJmb2</recordid><startdate>19840601</startdate><enddate>19840601</enddate><creator>BOPP, BERNARD W.</creator><general>The Astronomical Society of the Pacific</general><scope>CYE</scope><scope>CYI</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19840601</creationdate><title>EMISSION LINES IN THE SPECTRA OF THE RV TAURI STARS U MONOCEROTIS AND AC HERCULIS</title><author>BOPP, BERNARD W.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c259t-7586bafd12230ad0cebe913c01252689dc97b8bb44052dcc2dee23b6bf6bd2173</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1984</creationdate><topic>Absorption spectra</topic><topic>Astrophysics</topic><topic>Emission spectra</topic><topic>Light curves</topic><topic>Line spectra</topic><topic>Radial velocity</topic><topic>RV Tauri variables</topic><topic>Spectroscopy</topic><topic>Stellar spectra</topic><topic>Visible spectrum</topic><topic>Wavelengths</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>BOPP, BERNARD W.</creatorcontrib><collection>NASA Scientific and Technical Information</collection><collection>NASA Technical Reports Server</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>BOPP, BERNARD W.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>EMISSION LINES IN THE SPECTRA OF THE RV TAURI STARS U MONOCEROTIS AND AC HERCULIS</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1984-06-01</date><risdate>1984</risdate><volume>96</volume><issue>580</issue><spage>432</spage><epage>436</epage><pages>432-436</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><abstract>Strong metallic emission lines have been observed in the spectra of the RV Tauri stars U Mon and AC Her near recent light minima. While these two variables differ in a number of significant respects, the metallic emission spectra are quite similar, resembling the emission that we have previously reported as present in the spectrum of R Sct at a deep minimum. The data appear to support Baird's shock-wave model for the spectral behavior of RV Tauri stars.</abstract><cop>Legacy CDMS</cop><pub>The Astronomical Society of the Pacific</pub><doi>10.1086/131359</doi><tpages>5</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-6280 |
| ispartof | Publications of the Astronomical Society of the Pacific, 1984-06, Vol.96 (580), p.432-436 |
| issn | 0004-6280 1538-3873 |
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| source | IOP Publishing Journals; JSTOR Archive Collection A-Z Listing; NASA Technical Reports Server; EZB-FREE-00999 freely available EZB journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection |
| subjects | Absorption spectra Astrophysics Emission spectra Light curves Line spectra Radial velocity RV Tauri variables Spectroscopy Stellar spectra Visible spectrum Wavelengths |
| title | EMISSION LINES IN THE SPECTRA OF THE RV TAURI STARS U MONOCEROTIS AND AC HERCULIS |
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