2018
DOI: 10.1007/s00410-018-1504-z
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Magma evolution beneath Bequia, Lesser Antilles, deduced from petrology of lavas and plutonic xenoliths

Abstract: General rightsThis document is made available in accordance with publisher policies. Please cite only the published version using the reference above. Full terms of use are available: http://www.bristol.ac.uk/pure/about/ebr-terms Vol.:(0123456789) 1 3Contributions to Mineralogy and Petrology (2018) AbstractExtrusive and intrusive igneous rocks represent different parts of a magmatic system and ultimately provide complementary information about the processes operating beneath volcanoes. To shed light on such… Show more

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Cited by 18 publications
(36 citation statements)
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“…The high water contents recorded in Statia MIs (0.1–9.1 wt% H 2 O) are consistent with high water contents measured in melt inclusions from Montserrat (Humphreys et al 2009 ; Cassidy et al 2015 ), Bequia (Camejo-Harry et al 2018 ) and Dominica (Balcone-Boissard et al 2018 ) up to 6.2, 7.8 and 8 wt% H 2 O, respectively. In addition, independent estimates of melt water contents using orthopyroxene in andesites from Soufrière Hills Volcano, Montserrat, suggest melt water concentrations of 6–9 wt% H 2 O (Edmonds et al 2016 ).…”
Section: Discussionsupporting
confidence: 79%
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“…The high water contents recorded in Statia MIs (0.1–9.1 wt% H 2 O) are consistent with high water contents measured in melt inclusions from Montserrat (Humphreys et al 2009 ; Cassidy et al 2015 ), Bequia (Camejo-Harry et al 2018 ) and Dominica (Balcone-Boissard et al 2018 ) up to 6.2, 7.8 and 8 wt% H 2 O, respectively. In addition, independent estimates of melt water contents using orthopyroxene in andesites from Soufrière Hills Volcano, Montserrat, suggest melt water concentrations of 6–9 wt% H 2 O (Edmonds et al 2016 ).…”
Section: Discussionsupporting
confidence: 79%
“…2 ) but share the same general mineral assemblages (Fig. 3 ) as those recorded on the other islands in the Lesser Antilles (Arculus and Wills 1980 ; Camejo-Harry et al 2018 ; Cooper et al 2016 ; Kiddle et al 2010 ; Melekhova et al 2017 , 2015 , 2019 ; Stamper et al 2014 ; Tollan et al 2012 ). Cumulate xenoliths are very coarse grained (≤ 1 cm) and dominated by unzoned calcic plagioclase and hornblende (Figs.…”
Section: Resultsmentioning
confidence: 54%
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