Absolute magnitude in the K band of carbon stars
The relationship between the absolute magnitude in the K band and the IRAS color index of (12)-(25) was derived for carbon stars in the solar neighborhood by kinematical analyses of the radial-velocity data and the newly published proper-motion data in the ACRS catalog. The mean absolute magnitude i...
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| Veröffentlicht in: | Publications of the Astronomical Society of Japan 1993-08, Vol.45 (4), p.587-593 |
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| container_title | Publications of the Astronomical Society of Japan |
| container_volume | 45 |
| creator | MIKAMI, T ISHIDA, K |
| description | The relationship between the absolute magnitude in the K band and the IRAS color index of (12)-(25) was derived for carbon stars in the solar neighborhood by kinematical analyses of the radial-velocity data and the newly published proper-motion data in the ACRS catalog. The mean absolute magnitude in the K band of carbon stars varies from -8.0 to -8.6 with increases of 0.1 to 0.6 in (12)-(25). This tendency indicates that the more luminous carbon stars have a thicker circumstellar dust shell. |
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The mean absolute magnitude in the K band of carbon stars varies from -8.0 to -8.6 with increases of 0.1 to 0.6 in (12)-(25). This tendency indicates that the more luminous carbon stars have a thicker circumstellar dust shell.</description><identifier>ISSN: 0004-6264</identifier><identifier>CODEN: PASJAC</identifier><language>eng</language><publisher>Tokyo: Maruzen</publisher><subject>Astronomy ; Carbon stars, s stars, and related types (c, s, r, and n) ; Earth, ocean, space ; Exact sciences and technology ; Stars ; Variable and peculiar stars (including novae)</subject><ispartof>Publications of the Astronomical Society of Japan, 1993-08, Vol.45 (4), p.587-593</ispartof><rights>1994 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=3893725$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>MIKAMI, T</creatorcontrib><creatorcontrib>ISHIDA, K</creatorcontrib><title>Absolute magnitude in the K band of carbon stars</title><title>Publications of the Astronomical Society of Japan</title><description>The relationship between the absolute magnitude in the K band and the IRAS color index of (12)-(25) was derived for carbon stars in the solar neighborhood by kinematical analyses of the radial-velocity data and the newly published proper-motion data in the ACRS catalog. The mean absolute magnitude in the K band of carbon stars varies from -8.0 to -8.6 with increases of 0.1 to 0.6 in (12)-(25). This tendency indicates that the more luminous carbon stars have a thicker circumstellar dust shell.</description><subject>Astronomy</subject><subject>Carbon stars, s stars, and related types (c, s, r, and n)</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Stars</subject><subject>Variable and peculiar stars (including novae)</subject><issn>0004-6264</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1993</creationdate><recordtype>article</recordtype><recordid>eNotzj1rwzAUhWENLTRN-x80lG6GK11JtscQ-kUDXbKba-sqcbHlVLKH_vsamuksD4f3RmwAwBROO3Mn7nP-BtDKVWojYNfmaVhmliOdYj8vnmUf5Xxm-Slbil5OQXaU2inKPFPKD-I20JD58bpbcXx9Oe7fi8PX28d-dyhiZW3h0CM7Q5UzgOisDxx8QBXa4LhCE1qowSmHyhr0TLpEHdYkr1ErrQG34vn_9pKmn4Xz3Ix97ngYKPK05Ebb2pag7QqfrpByR0NIFLs-N5fUj5R-G6xqLFf2B3yeSpE</recordid><startdate>199308</startdate><enddate>199308</enddate><creator>MIKAMI, T</creator><creator>ISHIDA, K</creator><general>Maruzen</general><scope>IQODW</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>199308</creationdate><title>Absolute magnitude in the K band of carbon stars</title><author>MIKAMI, T ; ISHIDA, K</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-n855-63d3e64a86403365dfefdf31fbf6e834fb09061631543dea2732f216d23212203</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1993</creationdate><topic>Astronomy</topic><topic>Carbon stars, s stars, and related types (c, s, r, and n)</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Stars</topic><topic>Variable and peculiar stars (including novae)</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>MIKAMI, T</creatorcontrib><creatorcontrib>ISHIDA, K</creatorcontrib><collection>Pascal-Francis</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Publications of the Astronomical Society of Japan</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>MIKAMI, T</au><au>ISHIDA, K</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Absolute magnitude in the K band of carbon stars</atitle><jtitle>Publications of the Astronomical Society of Japan</jtitle><date>1993-08</date><risdate>1993</risdate><volume>45</volume><issue>4</issue><spage>587</spage><epage>593</epage><pages>587-593</pages><issn>0004-6264</issn><coden>PASJAC</coden><abstract>The relationship between the absolute magnitude in the K band and the IRAS color index of (12)-(25) was derived for carbon stars in the solar neighborhood by kinematical analyses of the radial-velocity data and the newly published proper-motion data in the ACRS catalog. The mean absolute magnitude in the K band of carbon stars varies from -8.0 to -8.6 with increases of 0.1 to 0.6 in (12)-(25). This tendency indicates that the more luminous carbon stars have a thicker circumstellar dust shell.</abstract><cop>Tokyo</cop><pub>Maruzen</pub><tpages>7</tpages></addata></record> |
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| ispartof | Publications of the Astronomical Society of Japan, 1993-08, Vol.45 (4), p.587-593 |
| issn | 0004-6264 |
| language | eng |
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| source | EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
| subjects | Astronomy Carbon stars, s stars, and related types (c, s, r, and n) Earth, ocean, space Exact sciences and technology Stars Variable and peculiar stars (including novae) |
| title | Absolute magnitude in the K band of carbon stars |
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