Results 11 to 20 of about 272 (130)

Two-injection Scenario for the Hard X-Ray Excess Observed in Mrk 421

open access: yesThe Astrophysical Journal, 2023
An interesting result that was recently reported for Mrk 421 is the detection of a significant excess at hard X-ray energies, which could provide useful information to investigate particle acceleration and emission mechanisms in the relativistic jet ...
Wen Hu, Da-Hai Yan, Qiang-Lin Hu
doaj   +1 more source

Long-term X-Ray Outburst in the TeV-detected Blazar Mrk 501 in 2021–2022: Further Clues for the Emission and Unstable Processes

open access: yesThe Astrophysical Journal Supplement Series, 2023
This paper presents the results of a detailed X-ray timing and spectral analysis of Mrk 501, which are based mainly on the Swift data obtained during 2021 February–2022 December. The source showed strongly enhanced X-ray activity, characterized by a long-
B. Kapanadze, A. Gurchumelia, M. Aller
doaj   +1 more source

Polarization microvariability of BL Lacertae objects [PDF]

open access: yesAstronomy & Astrophysics, 2005
Fil: Andruchow, Ileana. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico Conicet - La Plata. Instituto de Astrofisica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronomicas y Geofisicas.
Andruchow, Ileana   +2 more
openaire   +2 more sources

An optical view of BL Lacertae objects [PDF]

open access: yesThe Astronomy and Astrophysics Review, 2014
44 pages, 21 figure, to appear in The Astronomy and Astrophysics ...
Falomo, Renato   +2 more
openaire   +2 more sources

Radio Polarization of BL Lacertae Objects [PDF]

open access: yesPublications of the Astronomical Society of Japan, 2006
In the present work, using the data base of the University of Michigan Radio Astronomy Observatory (UMRAO) at three radio frequencies (4.8 GHz, 8GHZ, and 14.5 GHz), we studied the polarization properties for 47 BL Lacertae objects: 38 radio selected BL Lac objects, 7 X-ray selected BL Lac objects, and two inter-middle objects (Mkn 421 and Mkn 501), and
Fan, Jun-Hui   +8 more
openaire   +2 more sources

ZBLLAC: A Spectroscopic Database of BL Lacertae Objects [PDF]

open access: yesThe Astrophysical Journal Supplement Series, 2020
Abstract This paper describes the database of optical spectra of BL Lacertae (BLL) objects (Z BLL objects) available at https://web.oapd.inaf.it/zbllac/. At present, it contains calibrated spectra for 295 BLL. For about 35% of them, we report a firm measure of redshift z, while for 35 sources we set a lower limit on z based on the ...
Marco Landoni   +3 more
openaire   +2 more sources

Gamma-ray Emission and Variability Processes in High-Energy-Peaked BL Lacertae Objects

open access: yesUniverse, 2023
BL Lac objects are active galactic nuclei notable for a beamed nonthermal radiation, which is generated in one of the relativistic jets forming a small angle to the observer’s line-of-sight.
Bidzina Kapanadze
doaj   +1 more source

Power for dry BL Lacertae objects [PDF]

open access: yesAstronomy & Astrophysics, 2009
4 pages, 3 figures, accepted by A& ...
Paggi, A.   +3 more
openaire   +2 more sources

Polarization and Variations of BL Lacertae Objects [PDF]

open access: yesPublications of the Astronomical Society of Japan, 2001
Abstract BL Lacertae objects are an extreme subclass of AGNs showing rapid and large-amplitude variability, high and variable polarization, and core-dominated radio emissions. If a strong beaming effect is the cause of the extreme observation properties, one would expect that these properties would be correlated with each other. Based on
Cheng, KS, Fan, JH, Zhang, L
openaire   +3 more sources

BL Lacertae objects as an evolutionary population [PDF]

open access: yesSymposium - International Astronomical Union, 1986
If the BL Lac Objects are active nuclei with a beamed component that is dominant when directed at us, their observed luminosity function must comprise a flat faint branch: N(L)dL ∝ L1+1/pdL with p=4.5 (Urry and Shafer 1984). If this is flatter than the LF NP(L) of the parent objects at equal observed L, then we expect the counts of BL Lacs to flatten ...
A. Cavaliere, E. Giallongo, F. Vagnetti
openaire   +1 more source

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