Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7250
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dc.contributor.authorManoj, P-
dc.contributor.authorVig, S-
dc.contributor.authorMaheswar, G-
dc.contributor.authorKamath, U. S-
dc.date.accessioned2020-11-19T13:41:54Z-
dc.date.available2020-11-19T13:41:54Z-
dc.date.issued2016-12-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 37, No. 4, 38en_US
dc.identifier.issn0973-7758-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/7250-
dc.descriptionOpen Access © Indian Academy of Sciences http://www.ias.ac.in/describe/article/joaa/037/04/0038en_US
dc.description.abstractStars and planetary systems are formed out of molecular clouds in the interstellar medium. Although the sequence of steps involved in star formation are generally known, a comprehensive theory which describes the details of the processes that drive formation of stars is still missing. The Square Kilometre Array (SKA), with its unprecedented sensitivity and angular resolution, will play a major role in filling these gaps in our understanding. In this article, we present a few science cases that the Indian star formation community is interested in pursuing with SKA, which include investigation of AU-sized structures in the neutral ISM, the origin of thermal and non-thermal radio jets from protostars and the accretion history of protostars, and formation of massive stars and their effect on the surrounding medium.en_US
dc.language.isoenen_US
dc.publisherIndian Academy of Sciencesen_US
dc.subjectHII regionsen_US
dc.subjectISM: jets and outflowsen_US
dc.subjectISM: structureen_US
dc.subjectStars: formationen_US
dc.subjectStars: protostarsen_US
dc.titleInterstellar medium and star formation studies with the square kilometre arrayen_US
dc.typeArticleen_US
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