Published 1985
| Version v1
Report
Detection of Ni 2 lambda 7378 in six Seyfert galaxies
Description
A line due to Ni 2 7378 in the Seyfert galaxies NGC 1068, 2110, 3227, 4151, 5506, and Arp 102 B was detected. The average Ni abundance is about 2 times solar, which is 5 times less than in the filaments of the Crab Nebula. This argues for nucleosynthetic processing in the latter. The Ni 2 line is spatially revolved in NGC 1068, and shows at least a factor of 4 enhancement in the Ni abundance away from the nucleus. The off-nuclear abundance of Ni in NGC 1068 approaches that of the Crab, which strongly suggests that type supernovae enriched the off-nuclear gas clouds
Availability note (English)
Available from NTIS, PC A02/MF A01.Additional details
Publishing Information
- Imprint Pagination
- 20 p.
- Report number
- N--86-14205
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17048878
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Numerical Data, Non-conventional Literature
- Descriptors DEI
- CHEMICAL COMPOSITION; CRAB NEBULA; DETECTION; EXPERIMENTAL DATA; NICKEL; NUCLEOSYNTHESIS; RED SHIFT; SEYFERT GALAXIES; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; COSMIC RADIO SOURCES; DATA; ELEMENTS; ERUPTIVE VARIABLE STARS; GALAXIES; INFORMATION; METALS; NEBULAE; NUMERICAL DATA; STARS; SUPERNOVA REMNANTS; SYNTHESIS; TRANSITION ELEMENTS; VARIABLE STARS