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Please use this identifier to cite or link to this item: http://cmuir.cmu.ac.th/jspui/handle/6653943832/57196
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dc.contributor.authorA. Richichien_US
dc.contributor.authorO. Tasuyaen_US
dc.contributor.authorP. Irawatien_US
dc.contributor.authorR. K. Yadaven_US
dc.date.accessioned2018-09-05T03:36:23Z-
dc.date.available2018-09-05T03:36:23Z-
dc.date.issued2017-12-01en_US
dc.identifier.issn00046256en_US
dc.identifier.other2-s2.0-85039426792en_US
dc.identifier.other10.3847/1538-3881/aa9068en_US
dc.identifier.urihttps://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85039426792&origin=inwarden_US
dc.identifier.urihttp://cmuir.cmu.ac.th/jspui/handle/6653943832/57196-
dc.description.abstract© 2017. The American Astronomical Society. All rights reserved.. We present the latest lunar occultation (LO) results obtained at the 2.4 m Thai National Telescope, continuing a program started in 2014. We report on 21 LO events for 20 stellar sources, yielding 7 binary stars, 1 angular diameter, and 1 star with extended circumstellar emission. These results, some of which are obtained for the first time, are discussed in the context of previous observations when available.en_US
dc.subjectEarth and Planetary Sciencesen_US
dc.subjectPhysics and Astronomyen_US
dc.titleFurther Lunar Occultations from the 2.4m Thai National Telescopeen_US
dc.typeJournalen_US
article.title.sourcetitleAstronomical Journalen_US
article.volume154en_US
article.stream.affiliationsOsservatorio Astrofisico Di Arcetrien_US
article.stream.affiliationsChiang Mai Universityen_US
article.stream.affiliationsNational Astronomical Research Institute of Thailanden_US
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