Results 131 to 140 of about 166 (155)

Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Resolving the hot and ionized Universe through the Sunyaev-Zeldovich effect. [PDF]

open access: yesOpen Res Eur
Di Mascolo L   +25 more
europepmc   +1 more source

Primordial black holes and their gravitational-wave signatures. [PDF]

open access: yesLiving Rev Relativ
Bagui E   +20 more
europepmc   +1 more source

Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Nakamura R   +24 more
europepmc   +1 more source

Radio Variability of Radio‐quiet and Radio‐loud Quasars [PDF]

open access: yesAstrophysical Journal, 2005
The majority of quasars are weak in their radio emission, with flux densities comparable to those in the optical, and energies far lower. A small fraction, about 10%, are hundreds to thousands of times stronger in the radio. Conventional wisdom holds that there are two classes of quasars, the radio quiets and radio louds, with a deficit of sources ...
Joseph Lehar, Heino Falcke
exaly   +6 more sources

Quasar feedback and the origin of radio emission in radio-quiet quasars [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2014
23 pages, accepted to ...
Nadia Zakamska   +2 more
exaly   +3 more sources

The radio emission in radio-quiet quasars: the VLBA perspective

open access: yesMonthly Notices of the Royal Astronomical Society, 2023
ABSTRACT The origin of the radio emission in radio-quiet quasars (RQQ) is not established yet. We present new VLBA observations at 1.6 and 4.9 GHz of 10 RQQ (9 detected), which together with published earlier observations of 8 RQQ (5 detected), forms a representative sample of 18 RQQ drawn from the Palomar–Green sample of low z (<
Ehud BÉHAR   +2 more
exaly   +4 more sources

Radio-loud and radio-quiet quasars observed by EXOSAT [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1992
We present results from the spectral analysis of EXOSAT data on 31 quasars, 18 radio-loud and 13 radio-quiet. Simple power-law models with fixed (Galactic) absorption give acceptable fits to the spectra obtained in the 2-10 keV band. Using the results from these fits we have compared the distributions of spectral indices α for the radio-loud and radio ...
Turner M J L, Saxton R D, M J L Turner
exaly   +2 more sources

Radio emission from radio-quiet quasars

Nature, 1980
In a search for radio emission from bright, optically selected quasars, we detected ∼50% of the quasars at 5 GHz. This radio detection rate is so much higher than that for faint quasars (
James Condon, S L O'Dell, O'Dell S L
exaly   +2 more sources

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