Loading…
OB-stars as extreme condition test beds
Massive stars are inherently extreme objects, in terms of radiation, mass loss, rotation, and sometimes also magnetic fields. Concentrating on a (personally biased) subset of processes related to pulsations, rapid rotation and its interplay with mass-loss, and the bi-stability mechanism, we will dis...
Saved in:
Published in: | Proceedings of the International Astronomical Union 2010-07, Vol.6 (S272), p.554-565 |
---|---|
Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | cdi_FETCH-LOGICAL-c393t-783c88450a6a9b82c5223c89e95060f767353327959777db027174a3d29cb303 |
---|---|
cites | cdi_FETCH-LOGICAL-c393t-783c88450a6a9b82c5223c89e95060f767353327959777db027174a3d29cb303 |
container_end_page | 565 |
container_issue | S272 |
container_start_page | 554 |
container_title | Proceedings of the International Astronomical Union |
container_volume | 6 |
creator | Puls, Joachim Sundqvist, Jon O. Rivero González, Jorge G. |
description | Massive stars are inherently extreme objects, in terms of radiation, mass loss, rotation, and sometimes also magnetic fields. Concentrating on a (personally biased) subset of processes related to pulsations, rapid rotation and its interplay with mass-loss, and the bi-stability mechanism, we will discuss how active (and normal) OB stars can serve as appropriate laboratories to provide further clues. |
doi_str_mv | 10.1017/S1743921311011434 |
format | article |
fullrecord | <record><control><sourceid>proquest_cross</sourceid><recordid>TN_cdi_proquest_miscellaneous_1367491800</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><cupid>10_1017_S1743921311011434</cupid><sourcerecordid>1367491800</sourcerecordid><originalsourceid>FETCH-LOGICAL-c393t-783c88450a6a9b82c5223c89e95060f767353327959777db027174a3d29cb303</originalsourceid><addsrcrecordid>eNp1kE9Lw0AQxRdRsFY_gLeAB71Ed3Y2md2jlvoHCj3Ye9hstpLSJHU3Af32bmgRUTzNzOP33gzD2CXwW-BAd69AErUAhDiCRHnEJqOUaiHg-LsHPGVnIWw4l7nCbMKulw9p6I0PiQmJ--i9a1xiu7aq-7prk96FPildFc7Zydpsg7s41ClbPc5Xs-d0sXx6md0vUosa-5QUWqVkxk1udKmEzYSIinY64zlfU06YIQrSmSaiquSC4mUGK6FtiRyn7GYfu_Pd-xCXF00drNtuTeu6IRSAOUkNio_o1S900w2-jcdFChShkjRSsKes70Lwbl3sfN0Y_1kAL8bPFX8-Fz148Jim9HX15n5E_-v6AmRxazo</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1318738470</pqid></control><display><type>article</type><title>OB-stars as extreme condition test beds</title><source>Cambridge Journals Online</source><creator>Puls, Joachim ; Sundqvist, Jon O. ; Rivero González, Jorge G.</creator><creatorcontrib>Puls, Joachim ; Sundqvist, Jon O. ; Rivero González, Jorge G.</creatorcontrib><description>Massive stars are inherently extreme objects, in terms of radiation, mass loss, rotation, and sometimes also magnetic fields. Concentrating on a (personally biased) subset of processes related to pulsations, rapid rotation and its interplay with mass-loss, and the bi-stability mechanism, we will discuss how active (and normal) OB stars can serve as appropriate laboratories to provide further clues.</description><identifier>ISSN: 1743-9213</identifier><identifier>EISSN: 1743-9221</identifier><identifier>DOI: 10.1017/S1743921311011434</identifier><language>eng</language><publisher>Cambridge, UK: Cambridge University Press</publisher><subject>Astronomy ; Astrophysics ; Contributed Papers ; Fluid mechanics ; Star & galaxy formation ; Stars & galaxies</subject><ispartof>Proceedings of the International Astronomical Union, 2010-07, Vol.6 (S272), p.554-565</ispartof><rights>Copyright © International Astronomical Union 2011</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c393t-783c88450a6a9b82c5223c89e95060f767353327959777db027174a3d29cb303</citedby><cites>FETCH-LOGICAL-c393t-783c88450a6a9b82c5223c89e95060f767353327959777db027174a3d29cb303</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.cambridge.org/core/product/identifier/S1743921311011434/type/journal_article$$EHTML$$P50$$Gcambridge$$H</linktohtml><link.rule.ids>314,780,784,27924,27925,72960</link.rule.ids></links><search><creatorcontrib>Puls, Joachim</creatorcontrib><creatorcontrib>Sundqvist, Jon O.</creatorcontrib><creatorcontrib>Rivero González, Jorge G.</creatorcontrib><title>OB-stars as extreme condition test beds</title><title>Proceedings of the International Astronomical Union</title><addtitle>Proc. IAU</addtitle><description>Massive stars are inherently extreme objects, in terms of radiation, mass loss, rotation, and sometimes also magnetic fields. Concentrating on a (personally biased) subset of processes related to pulsations, rapid rotation and its interplay with mass-loss, and the bi-stability mechanism, we will discuss how active (and normal) OB stars can serve as appropriate laboratories to provide further clues.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Contributed Papers</subject><subject>Fluid mechanics</subject><subject>Star & galaxy formation</subject><subject>Stars & galaxies</subject><issn>1743-9213</issn><issn>1743-9221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp1kE9Lw0AQxRdRsFY_gLeAB71Ed3Y2md2jlvoHCj3Ye9hstpLSJHU3Af32bmgRUTzNzOP33gzD2CXwW-BAd69AErUAhDiCRHnEJqOUaiHg-LsHPGVnIWw4l7nCbMKulw9p6I0PiQmJ--i9a1xiu7aq-7prk96FPildFc7Zydpsg7s41ClbPc5Xs-d0sXx6md0vUosa-5QUWqVkxk1udKmEzYSIinY64zlfU06YIQrSmSaiquSC4mUGK6FtiRyn7GYfu_Pd-xCXF00drNtuTeu6IRSAOUkNio_o1S900w2-jcdFChShkjRSsKes70Lwbl3sfN0Y_1kAL8bPFX8-Fz148Jim9HX15n5E_-v6AmRxazo</recordid><startdate>20100701</startdate><enddate>20100701</enddate><creator>Puls, Joachim</creator><creator>Sundqvist, Jon O.</creator><creator>Rivero González, Jorge G.</creator><general>Cambridge University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7XB</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>Q9U</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20100701</creationdate><title>OB-stars as extreme condition test beds</title><author>Puls, Joachim ; Sundqvist, Jon O. ; Rivero González, Jorge G.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c393t-783c88450a6a9b82c5223c89e95060f767353327959777db027174a3d29cb303</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Astronomy</topic><topic>Astrophysics</topic><topic>Contributed Papers</topic><topic>Fluid mechanics</topic><topic>Star & galaxy formation</topic><topic>Stars & galaxies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Puls, Joachim</creatorcontrib><creatorcontrib>Sundqvist, Jon O.</creatorcontrib><creatorcontrib>Rivero González, Jorge G.</creatorcontrib><collection>CrossRef</collection><collection>ProQuest Central (Corporate)</collection><collection>ProQuest Central (purchase pre-March 2016)</collection><collection>Science Database (Alumni Edition)</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni) (purchase pre-March 2016)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central</collection><collection>Advanced Technologies & Aerospace Database (1962 - current)</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>ProQuest Central Student</collection><collection>Aerospace Database</collection><collection>SciTech Premium Collection (Proquest) (PQ_SDU_P3)</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Science Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>ProQuest Central Basic</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Proceedings of the International Astronomical Union</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Puls, Joachim</au><au>Sundqvist, Jon O.</au><au>Rivero González, Jorge G.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>OB-stars as extreme condition test beds</atitle><jtitle>Proceedings of the International Astronomical Union</jtitle><addtitle>Proc. IAU</addtitle><date>2010-07-01</date><risdate>2010</risdate><volume>6</volume><issue>S272</issue><spage>554</spage><epage>565</epage><pages>554-565</pages><issn>1743-9213</issn><eissn>1743-9221</eissn><abstract>Massive stars are inherently extreme objects, in terms of radiation, mass loss, rotation, and sometimes also magnetic fields. Concentrating on a (personally biased) subset of processes related to pulsations, rapid rotation and its interplay with mass-loss, and the bi-stability mechanism, we will discuss how active (and normal) OB stars can serve as appropriate laboratories to provide further clues.</abstract><cop>Cambridge, UK</cop><pub>Cambridge University Press</pub><doi>10.1017/S1743921311011434</doi><tpages>12</tpages><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 1743-9213 |
ispartof | Proceedings of the International Astronomical Union, 2010-07, Vol.6 (S272), p.554-565 |
issn | 1743-9213 1743-9221 |
language | eng |
recordid | cdi_proquest_miscellaneous_1367491800 |
source | Cambridge Journals Online |
subjects | Astronomy Astrophysics Contributed Papers Fluid mechanics Star & galaxy formation Stars & galaxies |
title | OB-stars as extreme condition test beds |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-04T18%3A13%3A22IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=OB-stars%20as%20extreme%20condition%20test%20beds&rft.jtitle=Proceedings%20of%20the%20International%20Astronomical%20Union&rft.au=Puls,%20Joachim&rft.date=2010-07-01&rft.volume=6&rft.issue=S272&rft.spage=554&rft.epage=565&rft.pages=554-565&rft.issn=1743-9213&rft.eissn=1743-9221&rft_id=info:doi/10.1017/S1743921311011434&rft_dat=%3Cproquest_cross%3E1367491800%3C/proquest_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c393t-783c88450a6a9b82c5223c89e95060f767353327959777db027174a3d29cb303%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=1318738470&rft_id=info:pmid/&rft_cupid=10_1017_S1743921311011434&rfr_iscdi=true |