Study of Bubble Nebula using IUE high resolution Spectra
In this paper we have analyzed IUE high resolution spectra of the central star (BD+602522) of the Bubble nebula. We discuss velocities of the different regions along the line of sight to the bubble. We find that the Bubble Nebula is younger (by a factor of 100) than the exciting star suggesting that...
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | |
| container_volume | |
| creator | Anand, M. Y Kagali, B. A. I Murthy, Jayant |
| description | In this paper we have analyzed IUE high resolution spectra of the central
star (BD+602522) of the Bubble nebula. We discuss velocities of the different
regions along the line of sight to the bubble. We find that the Bubble Nebula
is younger (by a factor of 100) than the exciting star suggesting that either
the bubble is expanding into an inhomogenuous interstellar medium or that the
mechanics of the stellar wind are not fully understood. |
| doi_str_mv | 10.48550/arxiv.0903.2828 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_0903_2828</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>0903_2828</sourcerecordid><originalsourceid>FETCH-LOGICAL-a658-2b0eb0e00ab33756d548ffd2c70e9406c9833a709c7d4d4d300cf04a670115163</originalsourceid><addsrcrecordid>eNotj8tuwjAURL3pogL2XVX-gYSb-JklIF4SahfQdXTt2GApJciJq_L3PFrNSLM7mkPIWwE510LAFONv-MmhApaXutSvRO-H1Fxp5-k8GdM6-uFMapGmPpyPdPu1pKdwPNHo-q5NQ-jOdH9xdog4Ji8e295N_ndEDqvlYbHJdp_r7WK2y1AKnZUG3L0AaBhTQjaCa--b0ipwFQdpK80YKqisavg9DMB64CgVFIUoJBuR9z_s83l9ieEb47V-GNQPA3YDmWI_Fg</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Study of Bubble Nebula using IUE high resolution Spectra</title><source>arXiv.org</source><creator>Anand, M. Y ; Kagali, B. A. I ; Murthy, Jayant</creator><creatorcontrib>Anand, M. Y ; Kagali, B. A. I ; Murthy, Jayant</creatorcontrib><description>In this paper we have analyzed IUE high resolution spectra of the central
star (BD+602522) of the Bubble nebula. We discuss velocities of the different
regions along the line of sight to the bubble. We find that the Bubble Nebula
is younger (by a factor of 100) than the exciting star suggesting that either
the bubble is expanding into an inhomogenuous interstellar medium or that the
mechanics of the stellar wind are not fully understood.</description><identifier>DOI: 10.48550/arxiv.0903.2828</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies</subject><creationdate>2009-03</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/0903.2828$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.0903.2828$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Anand, M. Y</creatorcontrib><creatorcontrib>Kagali, B. A. I</creatorcontrib><creatorcontrib>Murthy, Jayant</creatorcontrib><title>Study of Bubble Nebula using IUE high resolution Spectra</title><description>In this paper we have analyzed IUE high resolution spectra of the central
star (BD+602522) of the Bubble nebula. We discuss velocities of the different
regions along the line of sight to the bubble. We find that the Bubble Nebula
is younger (by a factor of 100) than the exciting star suggesting that either
the bubble is expanding into an inhomogenuous interstellar medium or that the
mechanics of the stellar wind are not fully understood.</description><subject>Physics - Astrophysics of Galaxies</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2009</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotj8tuwjAURL3pogL2XVX-gYSb-JklIF4SahfQdXTt2GApJciJq_L3PFrNSLM7mkPIWwE510LAFONv-MmhApaXutSvRO-H1Fxp5-k8GdM6-uFMapGmPpyPdPu1pKdwPNHo-q5NQ-jOdH9xdog4Ji8e295N_ndEDqvlYbHJdp_r7WK2y1AKnZUG3L0AaBhTQjaCa--b0ipwFQdpK80YKqisavg9DMB64CgVFIUoJBuR9z_s83l9ieEb47V-GNQPA3YDmWI_Fg</recordid><startdate>20090316</startdate><enddate>20090316</enddate><creator>Anand, M. Y</creator><creator>Kagali, B. A. I</creator><creator>Murthy, Jayant</creator><scope>GOX</scope></search><sort><creationdate>20090316</creationdate><title>Study of Bubble Nebula using IUE high resolution Spectra</title><author>Anand, M. Y ; Kagali, B. A. I ; Murthy, Jayant</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a658-2b0eb0e00ab33756d548ffd2c70e9406c9833a709c7d4d4d300cf04a670115163</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2009</creationdate><topic>Physics - Astrophysics of Galaxies</topic><toplevel>online_resources</toplevel><creatorcontrib>Anand, M. Y</creatorcontrib><creatorcontrib>Kagali, B. A. I</creatorcontrib><creatorcontrib>Murthy, Jayant</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Anand, M. Y</au><au>Kagali, B. A. I</au><au>Murthy, Jayant</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Study of Bubble Nebula using IUE high resolution Spectra</atitle><date>2009-03-16</date><risdate>2009</risdate><abstract>In this paper we have analyzed IUE high resolution spectra of the central
star (BD+602522) of the Bubble nebula. We discuss velocities of the different
regions along the line of sight to the bubble. We find that the Bubble Nebula
is younger (by a factor of 100) than the exciting star suggesting that either
the bubble is expanding into an inhomogenuous interstellar medium or that the
mechanics of the stellar wind are not fully understood.</abstract><doi>10.48550/arxiv.0903.2828</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.0903.2828 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_0903_2828 |
| source | arXiv.org |
| subjects | Physics - Astrophysics of Galaxies |
| title | Study of Bubble Nebula using IUE high resolution Spectra |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-10T23%3A14%3A23IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Study%20of%20Bubble%20Nebula%20using%20IUE%20high%20resolution%20Spectra&rft.au=Anand,%20M.%20Y&rft.date=2009-03-16&rft_id=info:doi/10.48550/arxiv.0903.2828&rft_dat=%3Carxiv_GOX%3E0903_2828%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |