Please use this identifier to cite or link to this item: http://hdl.handle.net/2080/3510
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dc.contributor.authorSahoo, Abinash-
dc.contributor.authorPradhan, Ananta C-
dc.contributor.authorMurthy, J-
dc.date.accessioned2020-03-03T12:42:07Z-
dc.date.available2020-03-03T12:42:07Z-
dc.date.issued2020-02-
dc.identifier.citation38th Annual Meeting of Astronomical Society of India, IISER, Tirupati, 13-17 February 2020en_US
dc.identifier.urihttp://hdl.handle.net/2080/3510-
dc.descriptionCopyright belongs to proceedings publisheren_US
dc.description.abstractA model has been generated to calculate the interstellar radiation field (ISRF) in the interstellar medium (ISM) in UV (912 \AA - 3000 \AA) within few parsecs of the Sun, using stellar catalog from Hipparcos mission. Comparison of model with previous models and observation from TD-1 satellite shows a good agreement. We found that B type stars contribute mostly to the total ISRF and constitute $\sim$7\% of the total number of stars in our model at distances between 0 pc and 500 pc. Stars farther away than 500 pc from the Sun contribute very less to the total ISRF as a result of attenuation by dust.en_US
dc.subjectModellingen_US
dc.subjectInterstellar Radiation Fielden_US
dc.subjectUltravioleten_US
dc.subjectUVen_US
dc.titleModelling Interstellar Radiation Field in UVen_US
dc.typeArticleen_US
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