Possible pulsations of the M giant in MWC560
MWC 560 and other peculiar symbiotic binary, CH Cyg, have been classified as the prototypes of the new subclass of symbiotic systems - propellers, with accretion onto a magnetic white dwarf being the source of activity. The companion of the hot component in this model should demonstrate stellar wind...
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| creator | Frackowiak, Sylwia M Mikolajewski, Maciej Tomov, Toma |
| description | MWC 560 and other peculiar symbiotic binary, CH Cyg, have been classified as
the prototypes of the new subclass of symbiotic systems - propellers, with
accretion onto a magnetic white dwarf being the source of activity. The
companion of the hot component in this model should demonstrate stellar wind
with relatively high mass-loss. It can be expected rather a late AGB, Mira or
semiregular variable (SR) than any normal red giant.Our analysis performed for
the I band shows that the M giant probably belongs to such kind of stars and
pulsates with a period of about 5 months. |
| doi_str_mv | 10.48550/arxiv.astro-ph/0210447 |
| format | Article |
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the prototypes of the new subclass of symbiotic systems - propellers, with
accretion onto a magnetic white dwarf being the source of activity. The
companion of the hot component in this model should demonstrate stellar wind
with relatively high mass-loss. It can be expected rather a late AGB, Mira or
semiregular variable (SR) than any normal red giant.Our analysis performed for
the I band shows that the M giant probably belongs to such kind of stars and
pulsates with a period of about 5 months.</description><identifier>DOI: 10.48550/arxiv.astro-ph/0210447</identifier><language>eng</language><subject>Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Physics - Earth and Planetary Astrophysics ; Physics - High Energy Astrophysical Phenomena ; Physics - Instrumentation and Methods for Astrophysics ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2002-10</creationdate><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/astro-ph/0210447$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.astro-ph/0210447$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Frackowiak, Sylwia M</creatorcontrib><creatorcontrib>Mikolajewski, Maciej</creatorcontrib><creatorcontrib>Tomov, Toma</creatorcontrib><title>Possible pulsations of the M giant in MWC560</title><description>MWC 560 and other peculiar symbiotic binary, CH Cyg, have been classified as
the prototypes of the new subclass of symbiotic systems - propellers, with
accretion onto a magnetic white dwarf being the source of activity. The
companion of the hot component in this model should demonstrate stellar wind
with relatively high mass-loss. It can be expected rather a late AGB, Mira or
semiregular variable (SR) than any normal red giant.Our analysis performed for
the I band shows that the M giant probably belongs to such kind of stars and
pulsates with a period of about 5 months.</description><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Earth and Planetary Astrophysics</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2002</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotzr1qwzAUQGEtGUrSZ6iWbnVyJUu6yhhM_yChHQIdzVV0XQsc21huad--kGY62-ET4k7B2nhrYUPTT_peU56noRjbDWgFxuCNeHgfck6hYzl-dZnmNPRZDo2cW5YH-Zmon2Xq5eGjsg5WYtFQl_n22qU4Pj0eq5di__b8Wu32BeEWi5LNiZ0Fj9RYHzkCk9c-NluHGKwBZGVQRxcDKg8n7zG40rDT2plgVbkU9__bC7oep3Sm6be-4Ouxra_48g8FOkBF</recordid><startdate>20021019</startdate><enddate>20021019</enddate><creator>Frackowiak, Sylwia M</creator><creator>Mikolajewski, Maciej</creator><creator>Tomov, Toma</creator><scope>GOX</scope></search><sort><creationdate>20021019</creationdate><title>Possible pulsations of the M giant in MWC560</title><author>Frackowiak, Sylwia M ; Mikolajewski, Maciej ; Tomov, Toma</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a797-3e4ce65087af58ded0ea828df9677b5407e1472d6db7180c887b634e62264b513</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2002</creationdate><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Physics - Earth and Planetary Astrophysics</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Frackowiak, Sylwia M</creatorcontrib><creatorcontrib>Mikolajewski, Maciej</creatorcontrib><creatorcontrib>Tomov, Toma</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Frackowiak, Sylwia M</au><au>Mikolajewski, Maciej</au><au>Tomov, Toma</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Possible pulsations of the M giant in MWC560</atitle><date>2002-10-19</date><risdate>2002</risdate><abstract>MWC 560 and other peculiar symbiotic binary, CH Cyg, have been classified as
the prototypes of the new subclass of symbiotic systems - propellers, with
accretion onto a magnetic white dwarf being the source of activity. The
companion of the hot component in this model should demonstrate stellar wind
with relatively high mass-loss. It can be expected rather a late AGB, Mira or
semiregular variable (SR) than any normal red giant.Our analysis performed for
the I band shows that the M giant probably belongs to such kind of stars and
pulsates with a period of about 5 months.</abstract><doi>10.48550/arxiv.astro-ph/0210447</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - Astrophysics of Galaxies Physics - Cosmology and Nongalactic Astrophysics Physics - Earth and Planetary Astrophysics Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Physics - Solar and Stellar Astrophysics |
| title | Possible pulsations of the M giant in MWC560 |
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