Photometric search of orbital periods in symbiotic stars
We present UBVRI photometry of three symbiotic stars ZZ CMi, TX CVn and AG Peg carried out from 1997 to 2008 in Piwnice Observatory near Torun. To search orbital periods of these stars Fourier analysis was used. For two of them, TX CVn and AG Peg, we have confirmed the earlier known periods. For ZZ...
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 | Wiecek, M Mikolajewski, M Tomov, T Cikala, M Galan, C Majcher, A Swierczynski, E Wychudzki, P Rozanski, P Frackowiak, S Janowski, J. L Graczyk, D |
| description | We present UBVRI photometry of three symbiotic stars ZZ CMi, TX CVn and AG
Peg carried out from 1997 to 2008 in Piwnice Observatory near Torun. To search
orbital periods of these stars Fourier analysis was used. For two of them, TX
CVn and AG Peg, we have confirmed the earlier known periods. For ZZ CMi we
found a relatively short period 218.59 days. Assuming, that the orbital period
is twice longer (P=437.18 days), the double sine wave in the light curve can be
interpreted by ellipsoidal effect. |
| doi_str_mv | 10.48550/arxiv.1003.0608 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_1003_0608</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1003_0608</sourcerecordid><originalsourceid>FETCH-LOGICAL-a658-fef4227e38534b9af2ae6bf245db74dd1fdd926dbe8de3c5a93d8f863d8a5b2d3</originalsourceid><addsrcrecordid>eNotjz1rwzAURbV0KEn3TkV_wK6sr8hjCE1bCDRDdvPk90QEcRUkUZJ_n7jtcu9yOdzD2HMnWu2MEa-QL_Gn7YRQrbDCPTK3P6aaJqo5jrwQ5PHIU-Ap-1jhxM-UY8LC4zcv18nHVOdZhVyW7CHAqdDTfy_YYft22Hw0u6_3z81614A1rgkUtJQrUs4o7XsIEsj6ILVBv9KIXUDspUVPDkmNBnqFLjh7TzBeolqwlz_s7_PhnOME-TrMBsNsoG6860Id</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Photometric search of orbital periods in symbiotic stars</title><source>arXiv.org</source><creator>Wiecek, M ; Mikolajewski, M ; Tomov, T ; Cikala, M ; Galan, C ; Majcher, A ; Swierczynski, E ; Wychudzki, P ; Rozanski, P ; Frackowiak, S ; Janowski, J. L ; Graczyk, D</creator><creatorcontrib>Wiecek, M ; Mikolajewski, M ; Tomov, T ; Cikala, M ; Galan, C ; Majcher, A ; Swierczynski, E ; Wychudzki, P ; Rozanski, P ; Frackowiak, S ; Janowski, J. L ; Graczyk, D</creatorcontrib><description>We present UBVRI photometry of three symbiotic stars ZZ CMi, TX CVn and AG
Peg carried out from 1997 to 2008 in Piwnice Observatory near Torun. To search
orbital periods of these stars Fourier analysis was used. For two of them, TX
CVn and AG Peg, we have confirmed the earlier known periods. For ZZ CMi we
found a relatively short period 218.59 days. Assuming, that the orbital period
is twice longer (P=437.18 days), the double sine wave in the light curve can be
interpreted by ellipsoidal effect.</description><identifier>DOI: 10.48550/arxiv.1003.0608</identifier><language>eng</language><subject>Physics - Solar and Stellar Astrophysics</subject><creationdate>2010-03</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>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/1003.0608$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.1003.0608$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Wiecek, M</creatorcontrib><creatorcontrib>Mikolajewski, M</creatorcontrib><creatorcontrib>Tomov, T</creatorcontrib><creatorcontrib>Cikala, M</creatorcontrib><creatorcontrib>Galan, C</creatorcontrib><creatorcontrib>Majcher, A</creatorcontrib><creatorcontrib>Swierczynski, E</creatorcontrib><creatorcontrib>Wychudzki, P</creatorcontrib><creatorcontrib>Rozanski, P</creatorcontrib><creatorcontrib>Frackowiak, S</creatorcontrib><creatorcontrib>Janowski, J. L</creatorcontrib><creatorcontrib>Graczyk, D</creatorcontrib><title>Photometric search of orbital periods in symbiotic stars</title><description>We present UBVRI photometry of three symbiotic stars ZZ CMi, TX CVn and AG
Peg carried out from 1997 to 2008 in Piwnice Observatory near Torun. To search
orbital periods of these stars Fourier analysis was used. For two of them, TX
CVn and AG Peg, we have confirmed the earlier known periods. For ZZ CMi we
found a relatively short period 218.59 days. Assuming, that the orbital period
is twice longer (P=437.18 days), the double sine wave in the light curve can be
interpreted by ellipsoidal effect.</description><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNotjz1rwzAURbV0KEn3TkV_wK6sr8hjCE1bCDRDdvPk90QEcRUkUZJ_n7jtcu9yOdzD2HMnWu2MEa-QL_Gn7YRQrbDCPTK3P6aaJqo5jrwQ5PHIU-Ap-1jhxM-UY8LC4zcv18nHVOdZhVyW7CHAqdDTfy_YYft22Hw0u6_3z81614A1rgkUtJQrUs4o7XsIEsj6ILVBv9KIXUDspUVPDkmNBnqFLjh7TzBeolqwlz_s7_PhnOME-TrMBsNsoG6860Id</recordid><startdate>20100302</startdate><enddate>20100302</enddate><creator>Wiecek, M</creator><creator>Mikolajewski, M</creator><creator>Tomov, T</creator><creator>Cikala, M</creator><creator>Galan, C</creator><creator>Majcher, A</creator><creator>Swierczynski, E</creator><creator>Wychudzki, P</creator><creator>Rozanski, P</creator><creator>Frackowiak, S</creator><creator>Janowski, J. L</creator><creator>Graczyk, D</creator><scope>GOX</scope></search><sort><creationdate>20100302</creationdate><title>Photometric search of orbital periods in symbiotic stars</title><author>Wiecek, M ; Mikolajewski, M ; Tomov, T ; Cikala, M ; Galan, C ; Majcher, A ; Swierczynski, E ; Wychudzki, P ; Rozanski, P ; Frackowiak, S ; Janowski, J. L ; Graczyk, D</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a658-fef4227e38534b9af2ae6bf245db74dd1fdd926dbe8de3c5a93d8f863d8a5b2d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Wiecek, M</creatorcontrib><creatorcontrib>Mikolajewski, M</creatorcontrib><creatorcontrib>Tomov, T</creatorcontrib><creatorcontrib>Cikala, M</creatorcontrib><creatorcontrib>Galan, C</creatorcontrib><creatorcontrib>Majcher, A</creatorcontrib><creatorcontrib>Swierczynski, E</creatorcontrib><creatorcontrib>Wychudzki, P</creatorcontrib><creatorcontrib>Rozanski, P</creatorcontrib><creatorcontrib>Frackowiak, S</creatorcontrib><creatorcontrib>Janowski, J. L</creatorcontrib><creatorcontrib>Graczyk, D</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Wiecek, M</au><au>Mikolajewski, M</au><au>Tomov, T</au><au>Cikala, M</au><au>Galan, C</au><au>Majcher, A</au><au>Swierczynski, E</au><au>Wychudzki, P</au><au>Rozanski, P</au><au>Frackowiak, S</au><au>Janowski, J. L</au><au>Graczyk, D</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Photometric search of orbital periods in symbiotic stars</atitle><date>2010-03-02</date><risdate>2010</risdate><abstract>We present UBVRI photometry of three symbiotic stars ZZ CMi, TX CVn and AG
Peg carried out from 1997 to 2008 in Piwnice Observatory near Torun. To search
orbital periods of these stars Fourier analysis was used. For two of them, TX
CVn and AG Peg, we have confirmed the earlier known periods. For ZZ CMi we
found a relatively short period 218.59 days. Assuming, that the orbital period
is twice longer (P=437.18 days), the double sine wave in the light curve can be
interpreted by ellipsoidal effect.</abstract><doi>10.48550/arxiv.1003.0608</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.1003.0608 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_1003_0608 |
| source | arXiv.org |
| subjects | Physics - Solar and Stellar Astrophysics |
| title | Photometric search of orbital periods in symbiotic stars |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-01T09%3A31%3A35IST&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=Photometric%20search%20of%20orbital%20periods%20in%20symbiotic%20stars&rft.au=Wiecek,%20M&rft.date=2010-03-02&rft_id=info:doi/10.48550/arxiv.1003.0608&rft_dat=%3Carxiv_GOX%3E1003_0608%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 |