The blazar sequence and its physical understanding

E Prandini, G Ghisellini - Galaxies, 2022 - mdpi.com
Introduced in 1998 to attempt a first unified view of the broad-band emission properties of
blazars, the blazar sequence has been extensively used in the past 25 years to guide …

Neutrino-dominated accretion flows as the central engine of gamma-ray bursts

T Liu, WM Gu, B Zhang - New Astronomy Reviews, 2017 - Elsevier
Neutrino-dominated accretion flows (NDAFs) around rotating stellar-mass black holes (BHs)
are plausible candidates for the central engines of gamma-ray bursts (GRBs). NDAFs are …

Spectral properties of quasars from Sloan Digital Sky Survey data release 14: The catalog

S Rakshit, CS Stalin, J Kotilainen - The Astrophysical Journal …, 2020 - iopscience.iop.org
We present measurements of the spectral properties for a total of 526,265 quasars, out of
which 63% have a continuum signal-to-noise ratio> 3 pixel− 1, selected from the fourteenth …

LOFAR observations of galaxy clusters in HETDEX-Extraction and self-calibration of individual LOFAR targets

RJ Van Weeren, TW Shimwell, A Botteon… - Astronomy & …, 2021 - aanda.org
Diffuse cluster radio sources, in the form of radio halos and relics, reveal the presence of
cosmic rays and magnetic fields in the intracluster medium (ICM). These cosmic rays are …

The power of relativistic jets is larger than the luminosity of their accretion disks

G Ghisellini, F Tavecchio, L Maraschi, A Celotti… - Nature, 2014 - nature.com
Theoretical models for the production of relativistic jets from active galactic nuclei predict that
jet power arises from the spin and mass of the central supermassive black hole, as well as …

Black hole mass scaling relations for early-type galaxies. I. MBH–M*, sph and MBH–M*, gal

N Sahu, AW Graham, BL Davis - The Astrophysical Journal, 2019 - iopscience.iop.org
Analyzing a sample of 84 early-type galaxies (ETGs) with directly measured supermassive
black hole masses—nearly doubling the sample size of such galaxies with multicomponent …

LoTSS jellyfish galaxies-I. Radio tails in low redshift clusters

ID Roberts, RJ Van Weeren, SL McGee… - Astronomy & …, 2021 - aanda.org
Context. The cluster environment has a strong impact on galaxy star formation, as seen by
the fact that clusters host proportionally more red, passive galaxies relative to the field. Ram …

[图书][B] Statistics and analysis of scientific data

M Bonamente - 2017 - Springer
With the third edition of Statistics and Analysis of Scientific Data, I have continued to pursue
the goal of providing a textbook that is both mathematically sound and easy to use for …

Black Hole Mass Scaling Relations for Spiral Galaxies. I. MBH–M*, sph

BL Davis, AW Graham, E Cameron - The Astrophysical Journal, 2019 - iopscience.iop.org
The (supermassive black hole mass, MBH)–(bulge stellar mass, M, sph*) relation is,
obviously, derived using two quantities. We endeavor to provide accurate values for the …

Minute-timescale> 100 MeV γ-ray variability during the giant outburst of quasar 3C 279 observed by Fermi-LAT in 2015 June

M Ackermann, R Anantua, K Asano… - The Astrophysical …, 2016 - iopscience.iop.org
ABSTRACT On 2015 June 16, Fermi-LAT observed a giant outburst from the flat spectrum
radio quasar 3C 279 with a peak> 100 MeV flux of∼ 3.6× 10− 5 photons cm− 2 s− 1 …