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http://hdl.handle.net/2080/3510Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Sahoo, Abinash | - |
| dc.contributor.author | Pradhan, Ananta C | - |
| dc.contributor.author | Murthy, J | - |
| dc.date.accessioned | 2020-03-03T12:42:07Z | - |
| dc.date.available | 2020-03-03T12:42:07Z | - |
| dc.date.issued | 2020-02 | - |
| dc.identifier.citation | 38th Annual Meeting of Astronomical Society of India, IISER, Tirupati, 13-17 February 2020 | en_US |
| dc.identifier.uri | http://hdl.handle.net/2080/3510 | - |
| dc.description | Copyright belongs to proceedings publisher | en_US |
| dc.description.abstract | A 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.subject | Modelling | en_US |
| dc.subject | Interstellar Radiation Field | en_US |
| dc.subject | Ultraviolet | en_US |
| dc.subject | UV | en_US |
| dc.title | Modelling Interstellar Radiation Field in UV | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | Conference Papers | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 2020_38th-ASI-Meeting_ASahoo_Modelling.pdf | Poster | 1.97 MB | Adobe PDF | View/Open |
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