2024RNAAS...8...63K


Query : 2024RNAAS...8...63K

2024RNAAS...8...63K - Research Notes of the AAS, 8, 63 (2024/March-0)

Quasars versus Microquasars: Scaling and Particle Acceleration.

KATZ J.I.

Abstract (from CDS):

Quasars and microquasars both contain accreting black holes and power nonthermal double radio sources, but differ in more than their scales: Quasars are proportionally much more efficient accelerators of energetic electrons. The radio luminosity of the double radio sources associated with quasars, reflecting the long-time average of the particle acceleration power, is often 1%-30% of the quasar's bolometric luminosity; in microquasars the fraction is ≲10–5. This may be explained by the scaling of accretion disk parameters with the black hole mass.

Abstract Copyright: © 2024. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Quasars - Supermassive black holes - Stellar mass black holes

Simbad objects: 9

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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 3C 48 QSO 01 37 41.2996631208 +33 09 35.080388820   16.62 16.20     ~ 2820 2
2 3C 273 BLL 12 29 06.6998257176 +02 03 08.597629980   13.05 14.830 14.11   ~ 5811 1
3 V* V818 Sco LXB 16 19 55.0692669024 -15 38 25.017666540 11.60 12.40 11.1     Oev 1644 0
4 NAME Great Annihilator LXB 17 43 54.83 -29 44 42.6           ~ 674 1
5 V* V479 Sct HXB 18 26 15.0561548880 -14 50 54.247274304 12.02 12.23 11.27 11.04   ON6V((f))z 573 2
6 SS 433 HXB 19 11 49.5647697480 +04 58 57.827127648   16.854 14.643     A3/7I 2125 4
7 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2633 0
8 NAME Cyg A Sy2 19 59 28.35656837 +40 44 02.0972325   16.22 15.10     ~ 2375 2
9 V* V1521 Cyg HXB 20 32 25.78 +40 57 27.9           WN4/5-6/7 1942 2

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