An Atlas of Low-Resolution Near-Infrared Spectra of Normal Stars
We present spectra of O to M stars, luminosity classes V, III, and Ib in the wavelength range 5800-8900 Å, at approximately 15 Å resolution. We give identifications of the main spectral features and show that the stars follow well-defined morphological sequences in both temperature and luminosity. T...
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Veröffentlicht in: | Publications of the Astronomical Society of the Pacific 1993-07, Vol.105 (689), p.693-720 |
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creator | Torres-Dodgen, Ana V. Weaver, Wm. Bruce |
description | We present spectra of O to M stars, luminosity classes V, III, and Ib in the wavelength range 5800-8900 Å, at approximately 15 Å resolution. We give identifications of the main spectral features and show that the stars follow well-defined morphological sequences in both temperature and luminosity. This wavelength region and resolution, combined with the high sensitivity of silicon-based detectors, are very useful for spectral classification. |
doi_str_mv | 10.1086/133222 |
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Bruce</creator><creatorcontrib>Torres-Dodgen, Ana V. ; Weaver, Wm. Bruce</creatorcontrib><description>We present spectra of O to M stars, luminosity classes V, III, and Ib in the wavelength range 5800-8900 Å, at approximately 15 Å resolution. We give identifications of the main spectral features and show that the stars follow well-defined morphological sequences in both temperature and luminosity. This wavelength region and resolution, combined with the high sensitivity of silicon-based detectors, are very useful for spectral classification.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/133222</identifier><identifier>CODEN: PASPAU</identifier><language>eng</language><publisher>Chicago, IL: American Institute of Physics</publisher><subject>Astronomy ; Calibration ; Catalogues, atlases, databases, retrieval systems, etc ; Earth, ocean, space ; Exact sciences and technology ; Fundamental astronomy and astrophysics. 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Bruce</creatorcontrib><title>An Atlas of Low-Resolution Near-Infrared Spectra of Normal Stars</title><title>Publications of the Astronomical Society of the Pacific</title><description>We present spectra of O to M stars, luminosity classes V, III, and Ib in the wavelength range 5800-8900 Å, at approximately 15 Å resolution. We give identifications of the main spectral features and show that the stars follow well-defined morphological sequences in both temperature and luminosity. This wavelength region and resolution, combined with the high sensitivity of silicon-based detectors, are very useful for spectral classification.</description><subject>Astronomy</subject><subject>Calibration</subject><subject>Catalogues, atlases, databases, retrieval systems, etc</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</subject><subject>Line spectra</subject><subject>Luminosity classification</subject><subject>M stars</subject><subject>Stars</subject><subject>Stellar classification</subject><subject>Stellar luminosities</subject><subject>Stellar spectra</subject><subject>Variable stars</subject><subject>Wavelengths</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1993</creationdate><recordtype>article</recordtype><recordid>eNpFj01LxDAURYMoWEf9B0IX4i768tWmO8sw6kAZwdF1eZMm0KHTDElF_Pe2VHR1F--8yz2EXDO4Z6CzByYE5_yEJEwJTYXOxSlJAEDSjGs4Jxcx7gEY0wwS8lj2aTl0GFPv0sp_0Tcbffc5tL5PNxYDXfcuYLBNuj1aMwScuI0PB-zS7YAhXpIzh120V7-5IB9Pq_flC61en9fLsqKGgxyoUtoqrUEZ5RqXcw4CLCopbcMsgsasYEVujLSInKHG0cIIZXdNNn7uQCzI3dxrgo8xWFcfQ3vA8F0zqCfvevYewdsZPGI02I3re9PGP1pqngGf-m5mbB8HH_7PkGmAohA_8Rpekw</recordid><startdate>19930701</startdate><enddate>19930701</enddate><creator>Torres-Dodgen, Ana V.</creator><creator>Weaver, Wm. Bruce</creator><general>American Institute of Physics</general><general>University of Chicago Press</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19930701</creationdate><title>An Atlas of Low-Resolution Near-Infrared Spectra of Normal Stars</title><author>Torres-Dodgen, Ana V. ; Weaver, Wm. Bruce</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c204t-558e58805c5fdf722030ea544ed1ea08a69197cc4eaa21a8a133c35ebd658eb03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1993</creationdate><topic>Astronomy</topic><topic>Calibration</topic><topic>Catalogues, atlases, databases, retrieval systems, etc</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</topic><topic>Line spectra</topic><topic>Luminosity classification</topic><topic>M stars</topic><topic>Stars</topic><topic>Stellar classification</topic><topic>Stellar luminosities</topic><topic>Stellar spectra</topic><topic>Variable stars</topic><topic>Wavelengths</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Torres-Dodgen, Ana V.</creatorcontrib><creatorcontrib>Weaver, Wm. Bruce</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Torres-Dodgen, Ana V.</au><au>Weaver, Wm. Bruce</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>An Atlas of Low-Resolution Near-Infrared Spectra of Normal Stars</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1993-07-01</date><risdate>1993</risdate><volume>105</volume><issue>689</issue><spage>693</spage><epage>720</epage><pages>693-720</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><coden>PASPAU</coden><abstract>We present spectra of O to M stars, luminosity classes V, III, and Ib in the wavelength range 5800-8900 Å, at approximately 15 Å resolution. We give identifications of the main spectral features and show that the stars follow well-defined morphological sequences in both temperature and luminosity. This wavelength region and resolution, combined with the high sensitivity of silicon-based detectors, are very useful for spectral classification.</abstract><cop>Chicago, IL</cop><pub>American Institute of Physics</pub><doi>10.1086/133222</doi><tpages>28</tpages></addata></record> |
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source | IOP Publishing Journals; Jstor Complete Legacy; EZB-FREE-00999 freely available EZB journals; Institute of Physics (IOP) Journals - HEAL-Link; Alma/SFX Local Collection |
subjects | Astronomy Calibration Catalogues, atlases, databases, retrieval systems, etc Earth, ocean, space Exact sciences and technology Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations Line spectra Luminosity classification M stars Stars Stellar classification Stellar luminosities Stellar spectra Variable stars Wavelengths |
title | An Atlas of Low-Resolution Near-Infrared Spectra of Normal Stars |
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