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Time variations of the neutral hydrogen absorption spectrum of NGC 1275 (3C 84)

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/160398· OSTI ID:6371073
The neutral hydrogen absorption spectrum and total radio continuum flux density of NGC 1275 (3C 84) have been monitored for temporal changes over a 6-year period. The strengths of two (at 8114 and 8120 km s/sup -1/) of the three dominant features in the spectrum have increased as the total flux density of NGC 1275 increased, although not by the same proportion. The third feature at 8106 km s/sup -1/ has not varied. Assuming a constant optical depth, we can calculate the flux density of the variable component which is being absorbed by the hydrogen at 8114 and 8120 km s/sup -1/. We find a flux density of 4.1 +- 0.6 Jy for epoch 1974.4, in reasonable agreement with VLBI results for the very compact component of the radio source in NGC 1275. The hydrogen at 8106 km s/sup -1/ must be absorbing another, more extended component of the radio source that does not vary. High-resolution spectral-line observations with the Very Large Array (VLA) indicate that >92% of the absorption at 8106 km s/sup -1/ occurs in a region <1'' in size. This implies that the hydrogen at 8106 km s/sup -1/ absorbs radio continuum with a scale size between 0--01 and 1--0. This result is in agreement with findings by Romney.
Research Organization:
Research Laboratory of Electronics and Haystack Observatory, Massachusetts Institute of Technology, and Harvard-Smithsonian Center for Astrophysics
OSTI ID:
6371073
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 262:1; ISSN ASJOA
Country of Publication:
United States
Language:
English

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