The high-mass slope of the IMF-Reference-Cited by-同舟云学术

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The high-mass slope of the IMF

Published:2018-07-17 Issue:2 Volume:480 Page:2449-2465
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Parravano Antonio¹²^ORCID,Hollenbach David³,McKee Christopher F⁴

Affiliation:

1. Centro De Física Fundamental, Universidad de Los Andes, Mérida 5101a, Venezuela

2. Departamento de Teoría e Historia Economica, Universidad de Málaga, 29013 Málaga, Spain

3. SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA

4. Physics and Astronomy Departments, University of California at Berkeley, Berkeley, CA 94720, USA

Funder

National Aeronautics and Space Administration

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/2/2449/25459692/sty1944.pdf

Reference53 articles.

1. Exploring the IMF of star clusters: a joint SLUG and LEGUS effort

2. Kinematics and history of the solar neighbourhood revisited

3. Age–velocity dispersion relations and heating histories in disc galaxies

4. A NEW CATALOG OF H II REGIONS IN M31

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