Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/4750
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dc.contributor.authorSingh, Kulinder Pal-
dc.date.accessioned2023-08-16T18:27:38Z-
dc.date.available2023-08-16T18:27:38Z-
dc.date.issued2022-
dc.identifier.citationResonance, 27(6), 961-981.en_US
dc.identifier.urihttps://doi.org/10.1007/s12045-022-1391-5-
dc.identifier.urihttp://hdl.handle.net/123456789/4750-
dc.descriptionOnly IISER Mohali authors are available in the record.en_US
dc.description.abstractAstroSat, launched in 2015, has observed all kinds of objects in the universe in X-rays and UV light. These objects range from isolated stars to stars in clusters, binary stars with compact companions like neutron stars and black holes, star-forming regions in the galaxies, and supermassive black holes in active nuclei of galaxies. In addition, it has carried out deep surveys of certain parts of the sky, reaching the farthest and the faintest objects in those regions. In this second part of the article, I highlight some of the important results obtained using AstroSat in the first five years of its operation.en_US
dc.language.isoen_USen_US
dc.publisherSpringer Natureen_US
dc.subjectAstroSaten_US
dc.subjectHighlights of Scientificen_US
dc.titleAstroSat: II. Highlights of Scientific Results From 2015–2021en_US
dc.title.alternativeScience From AstroSaten_US
dc.typeArticleen_US
Appears in Collections:Research Articles

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