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Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/3258
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dc.contributor.authorSingh, K.P.-
dc.date.accessioned2020-12-21T06:24:40Z-
dc.date.available2020-12-21T06:24:40Z-
dc.date.issued2020-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 498(3) pp. 3658-3663.en_US
dc.identifier.other10.1093/mnras/staa2574-
dc.identifier.urihttps://academic.oup.com/mnras/article/498/3/3658/5896469-
dc.identifier.urihttp://hdl.handle.net/123456789/3258-
dc.descriptionOnly IISERM authors are available in the record.-
dc.description.abstractOur nearest stellar neighbour, Proxima Centauri, is a low-mass star with spectral type dM5.5 and hosting an Earth-like planet orbiting within its habitable zone. However, the habitability of the planet depends on the high-energy radiation of the chromospheric and coronal activity of the host star. We report the AstroSat, Chandra, and HST observation of Proxima Centauri carried out as part of the multiwavelength simultaneous observational campaign. Using the soft X-ray data, we probe the different activity states of the star. We investigate the coronal temperatures, emission measures and abundance. Finally, we compare our results with earlier observations of Proxima Centauri.en_US
dc.language.isoen_USen_US
dc.publisherOxford University Pressen_US
dc.subjectstars: activityen_US
dc.subjectstars: coronaeen_US
dc.subjectstars: individual: Proxima Centaurien_US
dc.subjectstars: late-typeen_US
dc.titleProxima Centauri - The nearest planet host observed simultaneously with AstroSat, Chandra, and HSTen_US
dc.typeArticleen_US
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