Black Hole Mass Scaling Relations for Early-Type Galaxies. I. M BH–M *, SPH and M BH–M *,Gal

Astrophysical Journal - United States
doi 10.3847/1538-4357/ab0f32
Full Text
Abstract

Available in full text

Date
Authors
Publisher

American Astronomical Society

Related search

Black Hole and Nuclear Cluster Scaling Relations: M Bh ∝ M Nc 2.7±0.7

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

A Consistent Set of Empirical Scaling Relations for Spiral Galaxies: The (V Max, M oM)–(σ 0, M BH, Φ) Relations

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2019English

Red QSOs in the M BH -M∗ Plane

Proceedings of the International Astronomical Union
AstrophysicsAstronomyPlanetary ScienceSpace
2013English

Statistical Study of M 51-Type Galaxies

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2001English

I&M in Navigation Systems [Framing I&M Topics]

IEEE Instrumentation and Measurement Magazine
Electronic EngineeringElectricalInstrumentation
2015English

Asymptotic Stability of Ass(M/I N M)

Proceedings of the American Mathematical Society
MathematicsApplied Mathematics
1979English

Waiting Time Distribution for the M∕M∕m Queue

IEE Proceedings - Communications
2003English

M. M. Delafosse

Nature
Multidisciplinary
1927English

Early-Type Galaxies in the Near-Infrared: 1.5–2.4 $\Mu{\rm M}$ Spectroscopy

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2024 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy