INFRARED SPECTROSCOPY OF SYMBIOTIC STARS. IX. D-TYPE SYMBIOTIC NOVAE
Time-series spectra of the near-infrared 1.6 mu m region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mass velocity for the Mira. The Miras in most D...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal 2013-06, Vol.770 (1), p.1-25 |
|---|---|
| Hauptverfasser: | , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 25 |
|---|---|
| container_issue | 1 |
| container_start_page | 1 |
| container_title | The Astrophysical journal |
| container_volume | 770 |
| creator | Hinkle, Kenneth H FEKEL, FRANCIS C Joyce, Richard R Wood, Peter |
| description | Time-series spectra of the near-infrared 1.6 mu m region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mass velocity for the Mira. The Miras in most D-symbiotic novae have descended from intermediate mass progenitors. The large amount of mass lost from the Mira combined with the massive white dwarf companion suggests that these systems are supernova candidates. However, timescales and the number of objects make these rare events. |
| doi_str_mv | 10.1088/0004-637X/770/1/28 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22127163</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1730058587</sourcerecordid><originalsourceid>FETCH-LOGICAL-c385t-c3fb922b12b158ac784344073d44e74a186118a1e6daf0e7b06f4e5b314589c53</originalsourceid><addsrcrecordid>eNqNkU9Lw0AQxRdRsFa_gKeAFy9pdvZPdnOMaaoBbUoSpT0t6XaDkbap2fTgtzehIh6F4Q3D_HiH9xC6BTwBLKWHMWauT8XSEwJ74BF5hkbAqXQZ5eIcjX6BS3Rl7cdwkiAYoWkyn2VhFk-dfBFHRZbmUbpYOenMyVcvD0laJJGTF2GWT5xkOXGmbrFaxH9-8_QtjK_RRVVurbn52WP0OouL6Ml9Th-TKHx2NZW867VaB4SsoR8uSy0ko4xhQTeMGcFKkD6ALMH4m7LCRqyxXzHD1xQYl4HmdIzuTr6N7Wpldd0Z_a6b_d7oThECRIBPe-r-RB3a5vNobKd2tdVmuy33pjlaBYJizCWX4h8oDsD3mY97lJxQ3TbWtqZSh7bele2XAqyGDtSQqRoiVn0HChSR9BsJP3Do</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1709166460</pqid></control><display><type>article</type><title>INFRARED SPECTROSCOPY OF SYMBIOTIC STARS. IX. D-TYPE SYMBIOTIC NOVAE</title><source>IOP Publishing Free Content</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>Hinkle, Kenneth H ; FEKEL, FRANCIS C ; Joyce, Richard R ; Wood, Peter</creator><creatorcontrib>Hinkle, Kenneth H ; FEKEL, FRANCIS C ; Joyce, Richard R ; Wood, Peter</creatorcontrib><description>Time-series spectra of the near-infrared 1.6 mu m region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mass velocity for the Mira. The Miras in most D-symbiotic novae have descended from intermediate mass progenitors. The large amount of mass lost from the Mira combined with the massive white dwarf companion suggests that these systems are supernova candidates. However, timescales and the number of objects make these rare events.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/770/1/28</identifier><language>eng</language><publisher>United States</publisher><subject>ABSORPTION SPECTROSCOPY ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Binary systems ; CARBON MONOXIDE ; DUSTS ; INFRARED SPECTRA ; Infrared spectroscopy ; Kinematics ; MASS ; MOLECULES ; NOVAE ; Progenitors (astrophysics) ; Pulsation ; PULSATIONS ; SCATTERING ; Spectra ; STAR EVOLUTION ; STELLAR WINDS ; SUPERNOVAE ; SYMBIOTIC STARS ; WHITE DWARF STARS</subject><ispartof>The Astrophysical journal, 2013-06, Vol.770 (1), p.1-25</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c385t-c3fb922b12b158ac784344073d44e74a186118a1e6daf0e7b06f4e5b314589c53</citedby><cites>FETCH-LOGICAL-c385t-c3fb922b12b158ac784344073d44e74a186118a1e6daf0e7b06f4e5b314589c53</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,778,782,883,27911,27912</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22127163$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Hinkle, Kenneth H</creatorcontrib><creatorcontrib>FEKEL, FRANCIS C</creatorcontrib><creatorcontrib>Joyce, Richard R</creatorcontrib><creatorcontrib>Wood, Peter</creatorcontrib><title>INFRARED SPECTROSCOPY OF SYMBIOTIC STARS. IX. D-TYPE SYMBIOTIC NOVAE</title><title>The Astrophysical journal</title><description>Time-series spectra of the near-infrared 1.6 mu m region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mass velocity for the Mira. The Miras in most D-symbiotic novae have descended from intermediate mass progenitors. The large amount of mass lost from the Mira combined with the massive white dwarf companion suggests that these systems are supernova candidates. However, timescales and the number of objects make these rare events.</description><subject>ABSORPTION SPECTROSCOPY</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Binary systems</subject><subject>CARBON MONOXIDE</subject><subject>DUSTS</subject><subject>INFRARED SPECTRA</subject><subject>Infrared spectroscopy</subject><subject>Kinematics</subject><subject>MASS</subject><subject>MOLECULES</subject><subject>NOVAE</subject><subject>Progenitors (astrophysics)</subject><subject>Pulsation</subject><subject>PULSATIONS</subject><subject>SCATTERING</subject><subject>Spectra</subject><subject>STAR EVOLUTION</subject><subject>STELLAR WINDS</subject><subject>SUPERNOVAE</subject><subject>SYMBIOTIC STARS</subject><subject>WHITE DWARF STARS</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqNkU9Lw0AQxRdRsFa_gKeAFy9pdvZPdnOMaaoBbUoSpT0t6XaDkbap2fTgtzehIh6F4Q3D_HiH9xC6BTwBLKWHMWauT8XSEwJ74BF5hkbAqXQZ5eIcjX6BS3Rl7cdwkiAYoWkyn2VhFk-dfBFHRZbmUbpYOenMyVcvD0laJJGTF2GWT5xkOXGmbrFaxH9-8_QtjK_RRVVurbn52WP0OouL6Ml9Th-TKHx2NZW867VaB4SsoR8uSy0ko4xhQTeMGcFKkD6ALMH4m7LCRqyxXzHD1xQYl4HmdIzuTr6N7Wpldd0Z_a6b_d7oThECRIBPe-r-RB3a5vNobKd2tdVmuy33pjlaBYJizCWX4h8oDsD3mY97lJxQ3TbWtqZSh7bele2XAqyGDtSQqRoiVn0HChSR9BsJP3Do</recordid><startdate>20130610</startdate><enddate>20130610</enddate><creator>Hinkle, Kenneth H</creator><creator>FEKEL, FRANCIS C</creator><creator>Joyce, Richard R</creator><creator>Wood, Peter</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20130610</creationdate><title>INFRARED SPECTROSCOPY OF SYMBIOTIC STARS. IX. D-TYPE SYMBIOTIC NOVAE</title><author>Hinkle, Kenneth H ; FEKEL, FRANCIS C ; Joyce, Richard R ; Wood, Peter</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c385t-c3fb922b12b158ac784344073d44e74a186118a1e6daf0e7b06f4e5b314589c53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>ABSORPTION SPECTROSCOPY</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Binary systems</topic><topic>CARBON MONOXIDE</topic><topic>DUSTS</topic><topic>INFRARED SPECTRA</topic><topic>Infrared spectroscopy</topic><topic>Kinematics</topic><topic>MASS</topic><topic>MOLECULES</topic><topic>NOVAE</topic><topic>Progenitors (astrophysics)</topic><topic>Pulsation</topic><topic>PULSATIONS</topic><topic>SCATTERING</topic><topic>Spectra</topic><topic>STAR EVOLUTION</topic><topic>STELLAR WINDS</topic><topic>SUPERNOVAE</topic><topic>SYMBIOTIC STARS</topic><topic>WHITE DWARF STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Hinkle, Kenneth H</creatorcontrib><creatorcontrib>FEKEL, FRANCIS C</creatorcontrib><creatorcontrib>Joyce, Richard R</creatorcontrib><creatorcontrib>Wood, Peter</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hinkle, Kenneth H</au><au>FEKEL, FRANCIS C</au><au>Joyce, Richard R</au><au>Wood, Peter</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>INFRARED SPECTROSCOPY OF SYMBIOTIC STARS. IX. D-TYPE SYMBIOTIC NOVAE</atitle><jtitle>The Astrophysical journal</jtitle><date>2013-06-10</date><risdate>2013</risdate><volume>770</volume><issue>1</issue><spage>1</spage><epage>25</epage><pages>1-25</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>Time-series spectra of the near-infrared 1.6 mu m region have been obtained for five of the six known D-type symbiotic novae. The spectra map the pulsation kinematics of the Mira component in the Mira-white dwarf binary system and provide the center-of-mass velocity for the Mira. The Miras in most D-symbiotic novae have descended from intermediate mass progenitors. The large amount of mass lost from the Mira combined with the massive white dwarf companion suggests that these systems are supernova candidates. However, timescales and the number of objects make these rare events.</abstract><cop>United States</cop><doi>10.1088/0004-637X/770/1/28</doi><tpages>25</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-637X |
| ispartof | The Astrophysical journal, 2013-06, Vol.770 (1), p.1-25 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_osti_scitechconnect_22127163 |
| source | IOP Publishing Free Content; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
| subjects | ABSORPTION SPECTROSCOPY ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Binary systems CARBON MONOXIDE DUSTS INFRARED SPECTRA Infrared spectroscopy Kinematics MASS MOLECULES NOVAE Progenitors (astrophysics) Pulsation PULSATIONS SCATTERING Spectra STAR EVOLUTION STELLAR WINDS SUPERNOVAE SYMBIOTIC STARS WHITE DWARF STARS |
| title | INFRARED SPECTROSCOPY OF SYMBIOTIC STARS. IX. D-TYPE SYMBIOTIC NOVAE |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-16T00%3A39%3A08IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=INFRARED%20SPECTROSCOPY%20OF%20SYMBIOTIC%20STARS.%20IX.%20D-TYPE%20SYMBIOTIC%20NOVAE&rft.jtitle=The%20Astrophysical%20journal&rft.au=Hinkle,%20Kenneth%20H&rft.date=2013-06-10&rft.volume=770&rft.issue=1&rft.spage=1&rft.epage=25&rft.pages=1-25&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.1088/0004-637X/770/1/28&rft_dat=%3Cproquest_osti_%3E1730058587%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1709166460&rft_id=info:pmid/&rfr_iscdi=true |