Evidence of a Bottom-Heavy Initial Mass Function in Massive Early-Type Galaxies From Near-Infrared Metal Lines

Astrophysical Journal - United States
doi 10.3847/1538-4357/aa8563
Full Text
Abstract

Available in full text

Date
Authors
Publisher

American Astronomical Society

Related search

Evidence for a Constant Initial Mass Function in Early-Type Galaxies Based on Their X-Ray Binary Populations,

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2014English

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

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2009English

Mass to Light Ratio, Initial Mass Function, and Chemical Evolution in Disk Galaxies

Publications of the Astronomical Society of Australia
AstrophysicsAstronomyPlanetary ScienceSpace
2004English

Emission Lines in Early-Type Galaxies: Active Nuclei or Stars?

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2011English

Multiple Star Formation to the Bottom of the Initial Mass Function

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

On the Buildup of Massive Early-Type Galaxies Atz$\la$ 1

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2010English

Near-Infrared Stellar Populations in the Metal-Poor, Dwarf Irregular Galaxies Sextans a and Leo A

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2018English

Near-Infrared Spectroscopy of Seyfert and Starburst Galaxies

Symposium - International Astronomical Union
1989English

The Frequency of Barred Spiral Galaxies in the Near-Infrared

Astronomical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2000English

Amanote Research

Note-taking for researchers

Follow Amanote

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

Privacy PolicyRefund Policy