Inverse Compton γ rays from Cyg X-3?
[Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
FABIAN, A. C. [verfasserIn] BLANDFORD, R. D. [verfasserIn] HATCHETT, S. P. [verfasserIn] |
|---|
| Format: |
E-Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
s.l.: Nature Publishing Group ; 1977 |
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| Umfang: |
2 |
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| Reproduktion: |
Nature Archives 1869 - 2009 |
|---|---|
| Übergeordnetes Werk: |
In: Nature |
| Übergeordnetes Werk: |
volume:266 ; year:1977 ; number:5602 ; month:00 ; pages:512-513 ; extent:2 |
| Links: |
|---|
| DOI / URN: |
10.1038/266512a0 |
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NLEJ234046775 |
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10.1038/266512a0 doi (DE-627)NLEJ234046775 DE-627 ger DE-627 rakwb eng FABIAN, A. C. verfasserin aut Inverse Compton γ rays from Cyg X-3? [s.l.] Nature Publishing Group 1977 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside the ... Nature Archives 1869 - 2009 BLANDFORD, R. D. verfasserin aut HATCHETT, S. P. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 266(1977), 5602, Seite 512-513 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:266 year:1977 number:5602 month:00 pages:512-513 extent:2 http://dx.doi.org/10.1038/266512a0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 266 1977 5602 0 512-513 2 |
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10.1038/266512a0 doi (DE-627)NLEJ234046775 DE-627 ger DE-627 rakwb eng FABIAN, A. C. verfasserin aut Inverse Compton γ rays from Cyg X-3? [s.l.] Nature Publishing Group 1977 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside the ... Nature Archives 1869 - 2009 BLANDFORD, R. D. verfasserin aut HATCHETT, S. P. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 266(1977), 5602, Seite 512-513 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:266 year:1977 number:5602 month:00 pages:512-513 extent:2 http://dx.doi.org/10.1038/266512a0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 266 1977 5602 0 512-513 2 |
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10.1038/266512a0 doi (DE-627)NLEJ234046775 DE-627 ger DE-627 rakwb eng FABIAN, A. C. verfasserin aut Inverse Compton γ rays from Cyg X-3? [s.l.] Nature Publishing Group 1977 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside the ... Nature Archives 1869 - 2009 BLANDFORD, R. D. verfasserin aut HATCHETT, S. P. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 266(1977), 5602, Seite 512-513 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:266 year:1977 number:5602 month:00 pages:512-513 extent:2 http://dx.doi.org/10.1038/266512a0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 266 1977 5602 0 512-513 2 |
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10.1038/266512a0 doi (DE-627)NLEJ234046775 DE-627 ger DE-627 rakwb eng FABIAN, A. C. verfasserin aut Inverse Compton γ rays from Cyg X-3? [s.l.] Nature Publishing Group 1977 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside the ... Nature Archives 1869 - 2009 BLANDFORD, R. D. verfasserin aut HATCHETT, S. P. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 266(1977), 5602, Seite 512-513 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:266 year:1977 number:5602 month:00 pages:512-513 extent:2 http://dx.doi.org/10.1038/266512a0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 266 1977 5602 0 512-513 2 |
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10.1038/266512a0 doi (DE-627)NLEJ234046775 DE-627 ger DE-627 rakwb eng FABIAN, A. C. verfasserin aut Inverse Compton γ rays from Cyg X-3? [s.l.] Nature Publishing Group 1977 2 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier [Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside the ... Nature Archives 1869 - 2009 BLANDFORD, R. D. verfasserin aut HATCHETT, S. P. verfasserin aut In Nature <London> London [u.a.] : Nature Publising Group, 1869 266(1977), 5602, Seite 512-513 (DE-627)NLEJ227682335 (DE-600)1413423-8 1476-4687 nnns volume:266 year:1977 number:5602 month:00 pages:512-513 extent:2 http://dx.doi.org/10.1038/266512a0 application/pdf Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-NTA GBV_NL_ARTICLE AR 266 1977 5602 0 512-513 2 |
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[Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside the ... |
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[Auszug] Modulated ? rays are most efficiently produced by injecting the relativistic electrons in such a region for the following reasons. The ? rays cannot be created too close to the X-ray source (Rx 1010 cm), or they would be destroyed by pair creation in ?-ray-X-ray collisions. Creation outside the ... |
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