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http://nopr.niscpr.res.in/handle/123456789/38077Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Durgapal, M. C. | - |
| dc.contributor.author | Gehlot, G. L. | - |
| dc.date.accessioned | 2016-12-02T06:48:27Z | - |
| dc.date.available | 2016-12-02T06:48:27Z | - |
| dc.date.issued | 1972-09 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/38077 | - |
| dc.description | 195-197 | en_US |
| dc.description.abstract | Exact internal solutions have been found in a massive sphere with two density distributions surrounded by matter of very low density. The presence of external matter of very low density changes the gravitational potential to such an extent that the redshift obtained is as high as z = 3. Further, the results obtained have been applied to quasars, explaining the broadening and the large redshifts of the spectral lines. | en_US |
| dc.language.iso | en_US | en_US |
| dc.publisher | NISCAIR-CSIR, India | en_US |
| dc.rights |  CC Attribution-Noncommercial-No Derivative Works 2.5 India | en_US |
| dc.source | IJRSP Vol.01(3) [September 1972] | en_US |
| dc.title | Spheres with Three Density Distributions & Redshift from Stellar Bodies | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.01(3) [September 1972] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 1(3) 195-197.pdf | 296.62 kB | Adobe PDF | View/Open |
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