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Interstellar medium and star formation studies with the square kilometre array

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dc.contributor.author Manoj, P
dc.contributor.author Vig, S
dc.contributor.author Maheswar, G
dc.contributor.author Kamath, U. S
dc.date.accessioned 2020-11-19T13:41:54Z
dc.date.available 2020-11-19T13:41:54Z
dc.date.issued 2016-12
dc.identifier.citation Journal of Astrophysics and Astronomy, Vol. 37, No. 4, 38 en_US
dc.identifier.issn 0973-7758
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7250
dc.description Open Access © Indian Academy of Sciences http://www.ias.ac.in/describe/article/joaa/037/04/0038 en_US
dc.description.abstract Stars 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.iso en en_US
dc.publisher Indian Academy of Sciences en_US
dc.subject HII regions en_US
dc.subject ISM: jets and outflows en_US
dc.subject ISM: structure en_US
dc.subject Stars: formation en_US
dc.subject Stars: protostars en_US
dc.title Interstellar medium and star formation studies with the square kilometre array en_US
dc.type Article en_US


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