Results 1 to 10 of about 277 (132)

Polarization microvariability of BL Lacertae objects [PDF]

open access: yesAstronomy and 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.
I Andruchow, G E Romero, S A Cellone
exaly   +3 more sources

Quasi-periodicities of BL Lacertae objects [PDF]

open access: yesAstronomy and Astrophysics, 2018
We review the reports of possible year-long quasi-periodicities of BL Lac objects in the γ-ray and optical bands, and present a homogeneous time analysis of the light curves of PKS2155−304, PG1553+113, and BL Lac. Based on results from a survey covering the entire Fermi γ-ray sky we have estimated the fraction of possible quasi-periodic BL Lac objects.
Angela Sandrinelli   +2 more
exaly   +4 more sources

VHE observations of BL Lacertae objects: 1995–2000

open access: yesNew Astronomy Reviews, 2004
The results of observations of 29 BL Lacertae objects taken with the Whipple Observatory 10 m gamma-ray Telescope between 1995 and 2000 are presented.
exaly   +3 more sources

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

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

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

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

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

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