Open AccessRapid optical variability in radio‐quiet QSOs
Author(s) -
Gupta Alok C.,
Sagar Ram,
Wiita Paul J.,
Chaubey U. S.,
Stalin C. S.
Publication year - 2000
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2000.03446.x
Subject(s) - qsos , physics , quiet , astrophysics , observatory , quasar , astronomy , accretion (finance) , accretion disc , active galactic nucleus , uttar pradesh , galaxy , socioeconomics , sociology
We report results of the observations at the Vainu Bappu Observatory and the Uttar Pradesh State Observatory of eight radio‐quiet quasi‐stellar objects (RQQSOs) during 1996–99. This is a part of our ongoing programme to search for intranight optical variability in RQQSOs. Additional evidence for very rapid variability in three of the five optically bright and very luminous RQQSOs we had observed earlier, 1049−006, 1444+408 and 1630+377, was found. Of the three newly observed RQQSOs, the data for 0043+039 are too noisy to allow conclusions about variability to be drawn, but 0748+294 and 0824+098 show strong hints of microvariability. We also present a summary of the results from our entire programme to date, which includes observations of 16 radio‐quiet QSOs and one radio‐weak QSO, and compare the general properties of rapid variability in radio‐quiet versus radio‐loud AGN as determined from our work and that of several other groups. Observations of this kind are likely to play a key role in understanding the relative contributions of accretion discs and relativistic plasma jets to rapid optical fluctuations of AGN.