The difference between radio-loud and radio-quiet active galaxies
AS Wilson, EJM Colbert - arXiv preprint astro-ph/9408005, 1994 - arxiv.org
The recent development of unified theories of active galactic nuclei (AGN) has indicated that
there are two physically distinct classes of these objects-radio-loud and radio-quiet. The …
there are two physically distinct classes of these objects-radio-loud and radio-quiet. The …
[HTML][HTML] Comparative analysis of the high-and low-ionization lines in the broad-line region of active galactic nuclei
P Marziani, JW Sulentic… - … Supplement v. 104 …, 1996 - adsabs.harvard.edu
Comparative Analysis of the High- and Low-Ionization Lines in the Broad-Line Reg ADS Classic
is now deprecated. It will be completely retired in October 2019. This page will automatically …
is now deprecated. It will be completely retired in October 2019. This page will automatically …
ASTRONOMY AND ASTROPHYSICS LIBRARY
A Burkert, MA Dopita, A Eckart, T Encrenaz… - 2008 - Springer
This is the second edition of my book Galaxy Formation. Many people liked the first edition
which appeared in 1998, just before the explosion of magnificent new data which have …
which appeared in 1998, just before the explosion of magnificent new data which have …
Cosmological formation of low-mass objects
We investigate the early formation of bound objects with masses comparable to the
cosmological Jeans mass (10^ 5 solar masses). We follow the growth of isolated spherically …
cosmological Jeans mass (10^ 5 solar masses). We follow the growth of isolated spherically …
[HTML][HTML] Electron acceleration and gamma-ray emission from blazars
S Inoue, F Takahara - Astrophysical Journal v. 463, p. 555, 1996 - adsabs.harvard.edu
Electron Acceleration and Gamma-Ray Emission from Blazars ADS Classic is now deprecated.
It will be completely retired in October 2019. This page will automatically redirect to the new …
It will be completely retired in October 2019. This page will automatically redirect to the new …
A central stellar remnant in Puppis A
R Petre, CM Becker, PF Winkler - The Astrophysical Journal, 1996 - iopscience.iop.org
ABSTRACT ROSAT observations of a feature in the center of the Puppis A supernova
remnant suggest that it is the stellar remnant of the supernova. This feature has been known …
remnant suggest that it is the stellar remnant of the supernova. This feature has been known …
Optical polarization in distant radio galaxies
A Cimatti, S di Serego-Alighieri… - Monthly Notices of …, 1993 - adsabs.harvard.edu
We review the optical polarization properties of radio galaxies with redshifts greater than 0.1.
We find a strong tendency for the E-vector to be either perpendicular or parallel to the radio …
We find a strong tendency for the E-vector to be either perpendicular or parallel to the radio …
Quasars, blazars, and gamma rays
CD Dermer, R Schlickeiser - Science, 1992 - science.org
Before the launch of the Compton Gamma Ray Observatory (CGRO), the only source of>
100-megaelectron volt (MeV) gamma radiation known outside our galaxy was the quasar 3C …
100-megaelectron volt (MeV) gamma radiation known outside our galaxy was the quasar 3C …
Spectroscopic identification of ten faint hard X-ray sources discovered by Chandra
We report optical spectroscopic identifications of 10 hard (2–10 keV) X-ray selected sources
discovered by Chandra. The X-ray flux of the sources ranges between 1.5 and 25× 10 …
discovered by Chandra. The X-ray flux of the sources ranges between 1.5 and 25× 10 …
The 2dF galaxy redshift survey: clustering properties of radio galaxies
The clustering properties of local, S 1.4 GHz≥ 1 mJy, radio sources are investigated for a
sample of 820 objects drawn from the joint use of the Faint Images of the Radio Sky at 20 cm …
sample of 820 objects drawn from the joint use of the Faint Images of the Radio Sky at 20 cm …