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