PTF1 J191905.19+481506.2 - A Partially Eclipsing AM CVn System Discovered in the Palomar Transient Factory
We report on PTF1 J191905.19+481506.2, a newly discovered, partially eclipsing, outbursting AM CVn system found in the Palomar Transient Factory synoptic survey. This is only the second known eclipsing AM CVn system. We use high-speed photometric observations and phase-resolved spectroscopy to estab...
Gespeichert in:
| Veröffentlicht in: | arXiv.org 2014-02 |
|---|---|
| Hauptverfasser: | , , , , , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | arXiv.org |
| container_volume | |
| creator | Levitan, David Kupfer, Thomas Groot, Paul J Margon, Bruce Prince, Thomas A Kulkarni, Shrinivas R Hallinan, Gregg Harding, Leon K Kyne, Gillian Laher, Russ Ofek, Eran O Rutten, René G M Sesar, Branimir Surace, Jason |
| description | We report on PTF1 J191905.19+481506.2, a newly discovered, partially eclipsing, outbursting AM CVn system found in the Palomar Transient Factory synoptic survey. This is only the second known eclipsing AM CVn system. We use high-speed photometric observations and phase-resolved spectroscopy to establish an orbital period of 22.4559(3) min. We also present a long-term light curve and report on the normal and super-outbursts regularly seen in this system, including a super-outburst recurrence time of 36.8(4) d. We use the presence of the eclipse to place upper and lower limits on the inclination of the system and discuss the number of known eclipsing AM CVn systems versus what would be expected. |
| doi_str_mv | 10.48550/arxiv.1402.7129 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1402_7129</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2082890229</sourcerecordid><originalsourceid>FETCH-LOGICAL-a519-7a337258209dd50e65c21521d35fd64af473f796ea4e4c996caa1a0524c1683a3</originalsourceid><addsrcrecordid>eNotkEtLw0AURgdBsNTuXcmAS0mcufNIZllq64OKBYPbcJlMdEqa1JlUzL83ta7u5tyPwyHkirNU5kqxOww__jvlkkGacTBnZAJC8CSXABdkFuOWMQY6A6XEhGw3xYrTZ264YSrl5lbmXDGdAk3onG4w9B6bZqBL2_h99O0Hnb_QxXtL34bYux2999F23y64ivqW9p9u_Gm6HQZaBGyjd21PV2j7LgyX5LzGJrrZ_52SYrUsFo_J-vXhaTFfJ6i4STIUYnTLgZmqUsxpZYEr4JVQdaUl1jITdWa0Q-mkNUZbRI5MgbRc5wLFlFyfZv86lPvgR5uhPPYojz1G4OYE7EP3dXCxL7fdIbSjUgksh9wwGKlfUaJd4g</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2082890229</pqid></control><display><type>article</type><title>PTF1 J191905.19+481506.2 - A Partially Eclipsing AM CVn System Discovered in the Palomar Transient Factory</title><source>arXiv.org</source><source>Free E- Journals</source><creator>Levitan, David ; Kupfer, Thomas ; Groot, Paul J ; Margon, Bruce ; Prince, Thomas A ; Kulkarni, Shrinivas R ; Hallinan, Gregg ; Harding, Leon K ; Kyne, Gillian ; Laher, Russ ; Ofek, Eran O ; Rutten, René G M ; Sesar, Branimir ; Surace, Jason</creator><creatorcontrib>Levitan, David ; Kupfer, Thomas ; Groot, Paul J ; Margon, Bruce ; Prince, Thomas A ; Kulkarni, Shrinivas R ; Hallinan, Gregg ; Harding, Leon K ; Kyne, Gillian ; Laher, Russ ; Ofek, Eran O ; Rutten, René G M ; Sesar, Branimir ; Surace, Jason</creatorcontrib><description>We report on PTF1 J191905.19+481506.2, a newly discovered, partially eclipsing, outbursting AM CVn system found in the Palomar Transient Factory synoptic survey. This is only the second known eclipsing AM CVn system. We use high-speed photometric observations and phase-resolved spectroscopy to establish an orbital period of 22.4559(3) min. We also present a long-term light curve and report on the normal and super-outbursts regularly seen in this system, including a super-outburst recurrence time of 36.8(4) d. We use the presence of the eclipse to place upper and lower limits on the inclination of the system and discuss the number of known eclipsing AM CVn systems versus what would be expected.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1402.7129</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Eclipses ; Inclination ; Light curve ; Orbits ; Outbursts ; Photometry ; Physics - Solar and Stellar Astrophysics</subject><ispartof>arXiv.org, 2014-02</ispartof><rights>2014. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><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>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27902</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1402.7129$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1088/0004-637X/785/2/114$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Levitan, David</creatorcontrib><creatorcontrib>Kupfer, Thomas</creatorcontrib><creatorcontrib>Groot, Paul J</creatorcontrib><creatorcontrib>Margon, Bruce</creatorcontrib><creatorcontrib>Prince, Thomas A</creatorcontrib><creatorcontrib>Kulkarni, Shrinivas R</creatorcontrib><creatorcontrib>Hallinan, Gregg</creatorcontrib><creatorcontrib>Harding, Leon K</creatorcontrib><creatorcontrib>Kyne, Gillian</creatorcontrib><creatorcontrib>Laher, Russ</creatorcontrib><creatorcontrib>Ofek, Eran O</creatorcontrib><creatorcontrib>Rutten, René G M</creatorcontrib><creatorcontrib>Sesar, Branimir</creatorcontrib><creatorcontrib>Surace, Jason</creatorcontrib><title>PTF1 J191905.19+481506.2 - A Partially Eclipsing AM CVn System Discovered in the Palomar Transient Factory</title><title>arXiv.org</title><description>We report on PTF1 J191905.19+481506.2, a newly discovered, partially eclipsing, outbursting AM CVn system found in the Palomar Transient Factory synoptic survey. This is only the second known eclipsing AM CVn system. We use high-speed photometric observations and phase-resolved spectroscopy to establish an orbital period of 22.4559(3) min. We also present a long-term light curve and report on the normal and super-outbursts regularly seen in this system, including a super-outburst recurrence time of 36.8(4) d. We use the presence of the eclipse to place upper and lower limits on the inclination of the system and discuss the number of known eclipsing AM CVn systems versus what would be expected.</description><subject>Eclipses</subject><subject>Inclination</subject><subject>Light curve</subject><subject>Orbits</subject><subject>Outbursts</subject><subject>Photometry</subject><subject>Physics - Solar and Stellar Astrophysics</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><sourceid>GOX</sourceid><recordid>eNotkEtLw0AURgdBsNTuXcmAS0mcufNIZllq64OKBYPbcJlMdEqa1JlUzL83ta7u5tyPwyHkirNU5kqxOww__jvlkkGacTBnZAJC8CSXABdkFuOWMQY6A6XEhGw3xYrTZ264YSrl5lbmXDGdAk3onG4w9B6bZqBL2_h99O0Hnb_QxXtL34bYux2999F23y64ivqW9p9u_Gm6HQZaBGyjd21PV2j7LgyX5LzGJrrZ_52SYrUsFo_J-vXhaTFfJ6i4STIUYnTLgZmqUsxpZYEr4JVQdaUl1jITdWa0Q-mkNUZbRI5MgbRc5wLFlFyfZv86lPvgR5uhPPYojz1G4OYE7EP3dXCxL7fdIbSjUgksh9wwGKlfUaJd4g</recordid><startdate>20140228</startdate><enddate>20140228</enddate><creator>Levitan, David</creator><creator>Kupfer, Thomas</creator><creator>Groot, Paul J</creator><creator>Margon, Bruce</creator><creator>Prince, Thomas A</creator><creator>Kulkarni, Shrinivas R</creator><creator>Hallinan, Gregg</creator><creator>Harding, Leon K</creator><creator>Kyne, Gillian</creator><creator>Laher, Russ</creator><creator>Ofek, Eran O</creator><creator>Rutten, René G M</creator><creator>Sesar, Branimir</creator><creator>Surace, Jason</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20140228</creationdate><title>PTF1 J191905.19+481506.2 - A Partially Eclipsing AM CVn System Discovered in the Palomar Transient Factory</title><author>Levitan, David ; Kupfer, Thomas ; Groot, Paul J ; Margon, Bruce ; Prince, Thomas A ; Kulkarni, Shrinivas R ; Hallinan, Gregg ; Harding, Leon K ; Kyne, Gillian ; Laher, Russ ; Ofek, Eran O ; Rutten, René G M ; Sesar, Branimir ; Surace, Jason</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a519-7a337258209dd50e65c21521d35fd64af473f796ea4e4c996caa1a0524c1683a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Eclipses</topic><topic>Inclination</topic><topic>Light curve</topic><topic>Orbits</topic><topic>Outbursts</topic><topic>Photometry</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Levitan, David</creatorcontrib><creatorcontrib>Kupfer, Thomas</creatorcontrib><creatorcontrib>Groot, Paul J</creatorcontrib><creatorcontrib>Margon, Bruce</creatorcontrib><creatorcontrib>Prince, Thomas A</creatorcontrib><creatorcontrib>Kulkarni, Shrinivas R</creatorcontrib><creatorcontrib>Hallinan, Gregg</creatorcontrib><creatorcontrib>Harding, Leon K</creatorcontrib><creatorcontrib>Kyne, Gillian</creatorcontrib><creatorcontrib>Laher, Russ</creatorcontrib><creatorcontrib>Ofek, Eran O</creatorcontrib><creatorcontrib>Rutten, René G M</creatorcontrib><creatorcontrib>Sesar, Branimir</creatorcontrib><creatorcontrib>Surace, Jason</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</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>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Levitan, David</au><au>Kupfer, Thomas</au><au>Groot, Paul J</au><au>Margon, Bruce</au><au>Prince, Thomas A</au><au>Kulkarni, Shrinivas R</au><au>Hallinan, Gregg</au><au>Harding, Leon K</au><au>Kyne, Gillian</au><au>Laher, Russ</au><au>Ofek, Eran O</au><au>Rutten, René G M</au><au>Sesar, Branimir</au><au>Surace, Jason</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>PTF1 J191905.19+481506.2 - A Partially Eclipsing AM CVn System Discovered in the Palomar Transient Factory</atitle><jtitle>arXiv.org</jtitle><date>2014-02-28</date><risdate>2014</risdate><eissn>2331-8422</eissn><abstract>We report on PTF1 J191905.19+481506.2, a newly discovered, partially eclipsing, outbursting AM CVn system found in the Palomar Transient Factory synoptic survey. This is only the second known eclipsing AM CVn system. We use high-speed photometric observations and phase-resolved spectroscopy to establish an orbital period of 22.4559(3) min. We also present a long-term light curve and report on the normal and super-outbursts regularly seen in this system, including a super-outburst recurrence time of 36.8(4) d. We use the presence of the eclipse to place upper and lower limits on the inclination of the system and discuss the number of known eclipsing AM CVn systems versus what would be expected.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1402.7129</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2014-02 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_arxiv_primary_1402_7129 |
| source | arXiv.org; Free E- Journals |
| subjects | Eclipses Inclination Light curve Orbits Outbursts Photometry Physics - Solar and Stellar Astrophysics |
| title | PTF1 J191905.19+481506.2 - A Partially Eclipsing AM CVn System Discovered in the Palomar Transient Factory |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-07T22%3A40%3A12IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=PTF1%20J191905.19+481506.2%20-%20A%20Partially%20Eclipsing%20AM%20CVn%20System%20Discovered%20in%20the%20Palomar%20Transient%20Factory&rft.jtitle=arXiv.org&rft.au=Levitan,%20David&rft.date=2014-02-28&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1402.7129&rft_dat=%3Cproquest_arxiv%3E2082890229%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2082890229&rft_id=info:pmid/&rfr_iscdi=true |