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http://nopr.niscpr.res.in/handle/123456789/38016Full metadata record
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Durgapal, M. C. | - |
| dc.contributor.author | Gehlot, G. L. | - |
| dc.date.accessioned | 2016-12-01T09:30:57Z | - |
| dc.date.available | 2016-12-01T09:30:57Z | - |
| dc.date.issued | 1973-12 | - |
| dc.identifier.issn | 0975-105X (Online); 0367-8393 (Print) | - |
| dc.identifier.uri | http://nopr.niscair.res.in/handle/123456789/38016 | - |
| dc.description | 287-292 | en_US |
| dc.description.abstract | The effect of a layer of high density matter surrounding a spherical configuration has been studied. It has been shown that the maximum surface red-shift zs can be as large as 4.828. It is also shown that zs, and (radius) ratio increase when a sphere is surrounded by a layer of high density matter. Models of quasar proposed and the ratios (core mass/total mass) for some quasars with zs > 2 have been tabulated for two specific distributions of matter at the core. | 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.02(4) [December 1973] | en_US |
| dc.title | Massive Spheres in General Relativity & Large Gravitational of Quasars | en_US |
| dc.type | Article | en_US |
| Appears in Collections: | IJRSP Vol.02(4) [December 1973] | |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| IJRSP 2(4) 287-292.pdf | 884.96 kB | Adobe PDF | View/Open |
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