Three new pulsating sdB stars from the Edinburgh–Cape survey
We report the discovery of very rapid pulsations in three sdB stars from the Edinburgh–Cape blue object survey. The short periods, small amplitudes and multi-periodicity clearly establish these stars as members of the EC 14026 class. EC 11583−2708 has pulsation periods near 149, 144 and 114 s, thoug...
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creator | Kilkenny, D. Stobie, R. S. O'Donoghue, D. Koen, C. Hambly, N. MacGillivray, H. Lynas-Gray, A. E. |
description | We report the discovery of very rapid pulsations in three sdB stars from the Edinburgh–Cape blue object survey. The short periods, small amplitudes and multi-periodicity clearly establish these stars as members of the EC 14026 class. EC 11583−2708 has pulsation periods near 149, 144 and 114 s, though evidence is presented that the 149-s period is resolved into two periods at 148.87 and 148.55 s by the full photoelectric data set. The amplitudes of the detected variations are in the range 0.002–0.006 mag. The light variation of EC 20338−1925 is dominated by a period near 147 s with a very large amplitude for a variable sdB star (0.025 mag), though four other frequencies are detected with periods near 168, 151, 141 and 135 s and amplitudes in the range 0.002–0.005 mag. The third star, EC 09582−1137, displays a light curve which is virtually a textbook example of frequency beating, being produced by two pulsations of almost equal amplitude (∼0.008 mag) and periods near 136.0 and 151.2 s. |
doi_str_mv | 10.1111/j.1365-2966.2006.10065.x |
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S. ; O'Donoghue, D. ; Koen, C. ; Hambly, N. ; MacGillivray, H. ; Lynas-Gray, A. E.</creator><creatorcontrib>Kilkenny, D. ; Stobie, R. S. ; O'Donoghue, D. ; Koen, C. ; Hambly, N. ; MacGillivray, H. ; Lynas-Gray, A. E.</creatorcontrib><description>We report the discovery of very rapid pulsations in three sdB stars from the Edinburgh–Cape blue object survey. The short periods, small amplitudes and multi-periodicity clearly establish these stars as members of the EC 14026 class. EC 11583−2708 has pulsation periods near 149, 144 and 114 s, though evidence is presented that the 149-s period is resolved into two periods at 148.87 and 148.55 s by the full photoelectric data set. The amplitudes of the detected variations are in the range 0.002–0.006 mag. The light variation of EC 20338−1925 is dominated by a period near 147 s with a very large amplitude for a variable sdB star (0.025 mag), though four other frequencies are detected with periods near 168, 151, 141 and 135 s and amplitudes in the range 0.002–0.005 mag. The third star, EC 09582−1137, displays a light curve which is virtually a textbook example of frequency beating, being produced by two pulsations of almost equal amplitude (∼0.008 mag) and periods near 136.0 and 151.2 s.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1111/j.1365-2966.2006.10065.x</identifier><identifier>CODEN: MNRAA4</identifier><language>eng</language><publisher>Oxford, UK: Blackwell Publishing Ltd</publisher><subject>Astronomy ; Earth, ocean, space ; Exact sciences and technology ; Frequencies ; Pulsars ; Stars & galaxies ; stars: individual: EC 09582−1137 ; stars: individual: EC 11583−2708 ; stars: individual: EC 20338−1925 ; stars: oscillations ; stars: variables: other</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2006-04, Vol.367 (4), p.1603-1608</ispartof><rights>2006 The Authors. 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S.</creatorcontrib><creatorcontrib>O'Donoghue, D.</creatorcontrib><creatorcontrib>Koen, C.</creatorcontrib><creatorcontrib>Hambly, N.</creatorcontrib><creatorcontrib>MacGillivray, H.</creatorcontrib><creatorcontrib>Lynas-Gray, A. E.</creatorcontrib><title>Three new pulsating sdB stars from the Edinburgh–Cape survey</title><title>Monthly notices of the Royal Astronomical Society</title><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><description>We report the discovery of very rapid pulsations in three sdB stars from the Edinburgh–Cape blue object survey. The short periods, small amplitudes and multi-periodicity clearly establish these stars as members of the EC 14026 class. EC 11583−2708 has pulsation periods near 149, 144 and 114 s, though evidence is presented that the 149-s period is resolved into two periods at 148.87 and 148.55 s by the full photoelectric data set. The amplitudes of the detected variations are in the range 0.002–0.006 mag. The light variation of EC 20338−1925 is dominated by a period near 147 s with a very large amplitude for a variable sdB star (0.025 mag), though four other frequencies are detected with periods near 168, 151, 141 and 135 s and amplitudes in the range 0.002–0.005 mag. The third star, EC 09582−1137, displays a light curve which is virtually a textbook example of frequency beating, being produced by two pulsations of almost equal amplitude (∼0.008 mag) and periods near 136.0 and 151.2 s.</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Frequencies</subject><subject>Pulsars</subject><subject>Stars & galaxies</subject><subject>stars: individual: EC 09582−1137</subject><subject>stars: individual: EC 11583−2708</subject><subject>stars: individual: EC 20338−1925</subject><subject>stars: oscillations</subject><subject>stars: variables: other</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2006</creationdate><recordtype>article</recordtype><recordid>eNqNkd1q3DAQhUVpods07yAK7Z2dkbT6uwm0S5qEpFsISQi5EVpZznrrtR3Jbnbv-g59wzxJ7TikUFrSudAI9J0zGg5CmEBK-tpbpYQJnlAtREoBREr6g6ebF2jy9PASTQAYT5Qk5DV6E-MKAKaMignaP18G73Hl73DTldG2RXWDY_YJx9aGiPNQr3G79PggK6pFF26W9z9-zmzjcezCd799i17ltox-97HvoIvPB-ezo-T06-Hx7ONp4rimPMmYVsJ5mtl8obTNNaUuy0BaIZiwTnDCCZtyJ6aZZ4xZRmXmfJ4Dpf0SC8520IfRtwn1bedja9ZFdL4sbeXrLhqqQVKi2POgIsCplj347g9wVXeh6pcwFCTjUoF-HgICPaRGyIU6xuBz04RibcPWEDBDRmZlhijMEIUZMjIPGZlNL33_6G-js2UebOWK-FsvhSRaDSP2R-6uKP32v_3Nl_nZw7U3YKNB3TX_kCd_-14yqorY-s2TzoZvRkgmuTm6ujYn15cwV2eHZs5-AXgOwU8</recordid><startdate>200604</startdate><enddate>200604</enddate><creator>Kilkenny, D.</creator><creator>Stobie, R. S.</creator><creator>O'Donoghue, D.</creator><creator>Koen, C.</creator><creator>Hambly, N.</creator><creator>MacGillivray, H.</creator><creator>Lynas-Gray, A. E.</creator><general>Blackwell Publishing Ltd</general><general>Blackwell Science</general><general>Oxford University Press</general><scope>BSCLL</scope><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7U5</scope></search><sort><creationdate>200604</creationdate><title>Three new pulsating sdB stars from the Edinburgh–Cape survey</title><author>Kilkenny, D. ; Stobie, R. S. ; O'Donoghue, D. ; Koen, C. ; Hambly, N. ; MacGillivray, H. ; Lynas-Gray, A. 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S.</creatorcontrib><creatorcontrib>O'Donoghue, D.</creatorcontrib><creatorcontrib>Koen, C.</creatorcontrib><creatorcontrib>Hambly, N.</creatorcontrib><creatorcontrib>MacGillivray, H.</creatorcontrib><creatorcontrib>Lynas-Gray, A. E.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Solid State and Superconductivity Abstracts</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kilkenny, D.</au><au>Stobie, R. S.</au><au>O'Donoghue, D.</au><au>Koen, C.</au><au>Hambly, N.</au><au>MacGillivray, H.</au><au>Lynas-Gray, A. E.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Three new pulsating sdB stars from the Edinburgh–Cape survey</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><stitle>Monthly Notices of the Royal Astronomical Society</stitle><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><date>2006-04</date><risdate>2006</risdate><volume>367</volume><issue>4</issue><spage>1603</spage><epage>1608</epage><pages>1603-1608</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><coden>MNRAA4</coden><abstract>We report the discovery of very rapid pulsations in three sdB stars from the Edinburgh–Cape blue object survey. The short periods, small amplitudes and multi-periodicity clearly establish these stars as members of the EC 14026 class. EC 11583−2708 has pulsation periods near 149, 144 and 114 s, though evidence is presented that the 149-s period is resolved into two periods at 148.87 and 148.55 s by the full photoelectric data set. The amplitudes of the detected variations are in the range 0.002–0.006 mag. The light variation of EC 20338−1925 is dominated by a period near 147 s with a very large amplitude for a variable sdB star (0.025 mag), though four other frequencies are detected with periods near 168, 151, 141 and 135 s and amplitudes in the range 0.002–0.005 mag. The third star, EC 09582−1137, displays a light curve which is virtually a textbook example of frequency beating, being produced by two pulsations of almost equal amplitude (∼0.008 mag) and periods near 136.0 and 151.2 s.</abstract><cop>Oxford, UK</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1111/j.1365-2966.2006.10065.x</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Astronomy Earth, ocean, space Exact sciences and technology Frequencies Pulsars Stars & galaxies stars: individual: EC 09582−1137 stars: individual: EC 11583−2708 stars: individual: EC 20338−1925 stars: oscillations stars: variables: other |
title | Three new pulsating sdB stars from the Edinburgh–Cape survey |
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