Discovery of long-period variable stars in the very metal-poor globular cluster M15
We present a search for long-period variable (LPV) stars among giant branch stars in M15 which, at [Fe/H]∼−2.3, is one of the most metal-poor Galactic globular clusters. We use multicolour optical photometry from the 0.6-m Keele Thornton and 2-m Liverpool Telescopes. Variability of δV∼ 0.15 mag is d...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2010-07, Vol.405 (3), p.1711-1722 |
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creator | McDonald, I. van Loon, J. Th Dupree, A. K. Boyer, M. L. |
description | We present a search for long-period variable (LPV) stars among giant branch stars in M15 which, at [Fe/H]∼−2.3, is one of the most metal-poor Galactic globular clusters. We use multicolour optical photometry from the 0.6-m Keele Thornton and 2-m Liverpool Telescopes. Variability of δV∼ 0.15 mag is detected in K757 and K825 over unusually long time-scales of nearly a year, making them the most metal-poor LPVs found in a Galactic globular cluster. K825 is placed on the long secondary period sequence, identified for metal-rich LPVs, though no primary period is detectable. We discuss this variability in the context of dust production and stellar evolution at low metallicity, using additional spectra from the 6.5-m Magellan (Las Campanas) telescope. A lack of dust production, despite the presence of gaseous mass loss raises questions about the production of dust and the intracluster medium of this cluster. |
doi_str_mv | 10.1111/j.1365-2966.2010.16603.x |
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Th ; Dupree, A. K. ; Boyer, M. L.</creator><creatorcontrib>McDonald, I. ; van Loon, J. Th ; Dupree, A. K. ; Boyer, M. L.</creatorcontrib><description>We present a search for long-period variable (LPV) stars among giant branch stars in M15 which, at [Fe/H]∼−2.3, is one of the most metal-poor Galactic globular clusters. We use multicolour optical photometry from the 0.6-m Keele Thornton and 2-m Liverpool Telescopes. Variability of δV∼ 0.15 mag is detected in K757 and K825 over unusually long time-scales of nearly a year, making them the most metal-poor LPVs found in a Galactic globular cluster. K825 is placed on the long secondary period sequence, identified for metal-rich LPVs, though no primary period is detectable. We discuss this variability in the context of dust production and stellar evolution at low metallicity, using additional spectra from the 6.5-m Magellan (Las Campanas) telescope. 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Th</creatorcontrib><creatorcontrib>Dupree, A. K.</creatorcontrib><creatorcontrib>Boyer, M. L.</creatorcontrib><title>Discovery of long-period variable stars in the very metal-poor globular cluster M15</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 present a search for long-period variable (LPV) stars among giant branch stars in M15 which, at [Fe/H]∼−2.3, is one of the most metal-poor Galactic globular clusters. We use multicolour optical photometry from the 0.6-m Keele Thornton and 2-m Liverpool Telescopes. Variability of δV∼ 0.15 mag is detected in K757 and K825 over unusually long time-scales of nearly a year, making them the most metal-poor LPVs found in a Galactic globular cluster. K825 is placed on the long secondary period sequence, identified for metal-rich LPVs, though no primary period is detectable. We discuss this variability in the context of dust production and stellar evolution at low metallicity, using additional spectra from the 6.5-m Magellan (Las Campanas) telescope. A lack of dust production, despite the presence of gaseous mass loss raises questions about the production of dust and the intracluster medium of this cluster.</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>globular clusters: individual: M15</subject><subject>Metals</subject><subject>outflows</subject><subject>Stars & galaxies</subject><subject>stars: AGB and post-AGB</subject><subject>stars: late-type</subject><subject>stars: Population II</subject><subject>stars: variables: general</subject><subject>stars: winds</subject><subject>stars: winds, outflows</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2010</creationdate><recordtype>article</recordtype><recordid>eNp1kV2LEzEUhoMoWFf_QxDEq9QkJx_TG0HWjwpdBV1B9iZkMpl1ajoZk5m1_fdm2qUXirlJOOd5X07egxBmdMnKebVdMlCS8JVSS07nqlIUlvsHaHFuPEQLSkGSSjP2GD3JeUspFcDVAn1922UX73w64NjiEPtbMvjUxQbf2dTZOnicR5sy7no8_vD4SO78aAMZYkz4NsR6CjZhF6Y8-oSvmHyKHrU2ZP_s_r5A396_u75ck83nDx8v32yIE6CAgLdQubphfEUbC5rVrRASwFloVQvMaqc843zVVEKLWii38pVsnKJCtq6WcIFennyHFH9NPo9mVz7jQ7C9j1M2WgjFJXBayOd_kds4pb4MZyTTSopKVgV6cQ_Z7Gxok-1dl82Qup1NB1MGEaCBF-71ifvdBX849xk180LM1sy5mzl3My_EHBdi9ubq05fjsxjAySBOw3_k5B95UZGTqis57886m34apUFLs_5-Y_hG3qyv1doo-AOYvp39</recordid><startdate>201007</startdate><enddate>201007</enddate><creator>McDonald, I.</creator><creator>van Loon, J. 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L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4363-3ea38cbd1290da371bf44533ca3f6f31a7c6e1229d8474b46c9e85dc6045fcb53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2010</creationdate><topic>Astronomy</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>globular clusters: individual: M15</topic><topic>Metals</topic><topic>outflows</topic><topic>Stars & galaxies</topic><topic>stars: AGB and post-AGB</topic><topic>stars: late-type</topic><topic>stars: Population II</topic><topic>stars: variables: general</topic><topic>stars: winds</topic><topic>stars: winds, outflows</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>McDonald, I.</creatorcontrib><creatorcontrib>van Loon, J. Th</creatorcontrib><creatorcontrib>Dupree, A. K.</creatorcontrib><creatorcontrib>Boyer, M. L.</creatorcontrib><collection>Istex</collection><collection>Pascal-Francis</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>McDonald, I.</au><au>van Loon, J. Th</au><au>Dupree, A. K.</au><au>Boyer, M. L.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Discovery of long-period variable stars in the very metal-poor globular cluster M15</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>2010-07</date><risdate>2010</risdate><volume>405</volume><issue>3</issue><spage>1711</spage><epage>1722</epage><pages>1711-1722</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><coden>MNRAA4</coden><abstract>We present a search for long-period variable (LPV) stars among giant branch stars in M15 which, at [Fe/H]∼−2.3, is one of the most metal-poor Galactic globular clusters. We use multicolour optical photometry from the 0.6-m Keele Thornton and 2-m Liverpool Telescopes. Variability of δV∼ 0.15 mag is detected in K757 and K825 over unusually long time-scales of nearly a year, making them the most metal-poor LPVs found in a Galactic globular cluster. K825 is placed on the long secondary period sequence, identified for metal-rich LPVs, though no primary period is detectable. We discuss this variability in the context of dust production and stellar evolution at low metallicity, using additional spectra from the 6.5-m Magellan (Las Campanas) telescope. A lack of dust production, despite the presence of gaseous mass loss raises questions about the production of dust and the intracluster medium of this cluster.</abstract><cop>Oxford, UK</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1111/j.1365-2966.2010.16603.x</doi><tpages>12</tpages></addata></record> |
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subjects | Astronomy Earth, ocean, space Exact sciences and technology globular clusters: individual: M15 Metals outflows Stars & galaxies stars: AGB and post-AGB stars: late-type stars: Population II stars: variables: general stars: winds stars: winds, outflows |
title | Discovery of long-period variable stars in the very metal-poor globular cluster M15 |
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