Lynne A. Valencic, Kimberly A. Weaver, K. D. Kuntz, J. Cann, R. Pfeifle
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TUVO-21acq was found to have X-ray flux <jats:italic>F</jats:italic>\n <jats:sub>X</jats:sub>(0.4–3.0 keV) ∼ 1.3 × 10<jats:sup>−14</jats:sup> erg s<jats:sup>−1</jats:sup> cm<jats:sup>−2</jats:sup> and features similar to other quiescent dwarf novae, with X-ray luminosity <jats:italic>L</jats:italic>\n <jats:sub>X</jats:sub>(0.4–3.0 keV) ∼ 8 × 10<jats:sup>30</jats:sup> erg s<jats:sup>−1</jats:sup> and a white dwarf mass <jats:inline-formula>\n <jats:tex-math>\n\n</jats:tex-math>\n <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\" overflow=\"scroll\">\n <mml:msub>\n <mml:mrow>\n <mml:mi>M</mml:mi>\n </mml:mrow>\n <mml:mrow>\n <mml:mi>WD</mml:mi>\n </mml:mrow>\n </mml:msub>\n <mml:mo>=</mml:mo>\n <mml:msubsup>\n <mml:mrow>\n <mml:mn>0.78</mml:mn>\n </mml:mrow>\n <mml:mrow>\n <mml:mo>−</mml:mo>\n <mml:mn>0.27</mml:mn>\n </mml:mrow>\n <mml:mrow>\n <mml:mo>+</mml:mo>\n <mml:mn>0.37</mml:mn>\n </mml:mrow>\n </mml:msubsup>\n <mml:mspace width=\"0.25em\"/>\n <mml:msub>\n <mml:mrow>\n <mml:mi>M</mml:mi>\n </mml:mrow>\n <mml:mrow>\n <mml:mo>⊙</mml:mo>\n </mml:mrow>\n </mml:msub>\n </mml:math>\n <jats:inline-graphic xmlns:xlink=\"http://www.w3.org/1999/xlink\" xlink:href=\"paspad4592ieqn1.gif\" xlink:type=\"simple\"/>\n </jats:inline-formula>. Its UV/optical spectrum was variable between observations, possibly due to changes in the accretion disk or the visibility of the bright spot.</jats:p>","PeriodicalId":20820,"journal":{"name":"Publications of the Astronomical Society of the Pacific","volume":null,"pages":null},"PeriodicalIF":3.3000,"publicationDate":"2024-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"A Serendipitous Observation of the Recently Discovered Cataclysmic Variable TUVO-21acq\",\"authors\":\"Lynne A. Valencic, Kimberly A. Weaver, K. D. Kuntz, J. Cann, R. Pfeifle\",\"doi\":\"10.1088/1538-3873/ad4592\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"\\n <jats:p>The recently discovered non-magnetic cataclysmic variable TUVO-21acq was serendipitously observed in a quiescent state during an XMM-Newton observing campaign for the starburst galaxy NGC 4945. Data from this campaign was combined with archival serendipitous XMM observations to examine its X-ray and UV/optical characteristics. TUVO-21acq was found to have X-ray flux <jats:italic>F</jats:italic>\\n <jats:sub>X</jats:sub>(0.4–3.0 keV) ∼ 1.3 × 10<jats:sup>−14</jats:sup> erg s<jats:sup>−1</jats:sup> cm<jats:sup>−2</jats:sup> and features similar to other quiescent dwarf novae, with X-ray luminosity <jats:italic>L</jats:italic>\\n <jats:sub>X</jats:sub>(0.4–3.0 keV) ∼ 8 × 10<jats:sup>30</jats:sup> erg s<jats:sup>−1</jats:sup> and a white dwarf mass <jats:inline-formula>\\n <jats:tex-math>\\n\\n</jats:tex-math>\\n <mml:math xmlns:mml=\\\"http://www.w3.org/1998/Math/MathML\\\" overflow=\\\"scroll\\\">\\n <mml:msub>\\n <mml:mrow>\\n <mml:mi>M</mml:mi>\\n </mml:mrow>\\n <mml:mrow>\\n <mml:mi>WD</mml:mi>\\n </mml:mrow>\\n </mml:msub>\\n <mml:mo>=</mml:mo>\\n <mml:msubsup>\\n <mml:mrow>\\n <mml:mn>0.78</mml:mn>\\n </mml:mrow>\\n <mml:mrow>\\n <mml:mo>−</mml:mo>\\n <mml:mn>0.27</mml:mn>\\n </mml:mrow>\\n <mml:mrow>\\n <mml:mo>+</mml:mo>\\n <mml:mn>0.37</mml:mn>\\n </mml:mrow>\\n </mml:msubsup>\\n <mml:mspace width=\\\"0.25em\\\"/>\\n <mml:msub>\\n <mml:mrow>\\n <mml:mi>M</mml:mi>\\n </mml:mrow>\\n <mml:mrow>\\n <mml:mo>⊙</mml:mo>\\n </mml:mrow>\\n </mml:msub>\\n </mml:math>\\n <jats:inline-graphic xmlns:xlink=\\\"http://www.w3.org/1999/xlink\\\" xlink:href=\\\"paspad4592ieqn1.gif\\\" xlink:type=\\\"simple\\\"/>\\n </jats:inline-formula>. Its UV/optical spectrum was variable between observations, possibly due to changes in the accretion disk or the visibility of the bright spot.</jats:p>\",\"PeriodicalId\":20820,\"journal\":{\"name\":\"Publications of the Astronomical Society of the Pacific\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":3.3000,\"publicationDate\":\"2024-05-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Publications of the Astronomical Society of the Pacific\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1088/1538-3873/ad4592\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Publications of the Astronomical Society of the Pacific","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1088/1538-3873/ad4592","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
A Serendipitous Observation of the Recently Discovered Cataclysmic Variable TUVO-21acq
The recently discovered non-magnetic cataclysmic variable TUVO-21acq was serendipitously observed in a quiescent state during an XMM-Newton observing campaign for the starburst galaxy NGC 4945. Data from this campaign was combined with archival serendipitous XMM observations to examine its X-ray and UV/optical characteristics. TUVO-21acq was found to have X-ray flux FX(0.4–3.0 keV) ∼ 1.3 × 10−14 erg s−1 cm−2 and features similar to other quiescent dwarf novae, with X-ray luminosity LX(0.4–3.0 keV) ∼ 8 × 1030 erg s−1 and a white dwarf mass MWD=0.78−0.27+0.37M⊙. Its UV/optical spectrum was variable between observations, possibly due to changes in the accretion disk or the visibility of the bright spot.
期刊介绍:
The Publications of the Astronomical Society of the Pacific (PASP), the technical journal of the Astronomical Society of the Pacific (ASP), has been published regularly since 1889, and is an integral part of the ASP''s mission to advance the science of astronomy and disseminate astronomical information. The journal provides an outlet for astronomical results of a scientific nature and serves to keep readers in touch with current astronomical research. It contains refereed research and instrumentation articles, invited and contributed reviews, tutorials, and dissertation summaries.