Cluster kinematics and stellar rotation in NGC 419 with MUSE and adaptive optics-Reference-Cited by-同舟云学术

Cluster kinematics and stellar rotation in NGC 419 with MUSE and adaptive optics

Published:2018-07-24 Issue:2 Volume:480 Page:1689-1695
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Kamann S¹^ORCID,Bastian N¹,Husser T-O²,Martocchia S¹,Usher C¹^ORCID,den Brok M³,Dreizler S²,Kelz A³,Krajnović D³,Richard J⁴,Steinmetz M³,Weilbacher P M³

Affiliation:

1. Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK

2. Institut für Astrophysik, Georg-August Universität, Friedrich-Hund-Platz 1, D-37077Göttingen, Germany

3. Leibniz-Institute for Astrophysics (AIP), An der Sternwarte 16, D-14482 Potsdam, Germany

4. Univ Lyon, Univ Lyon1, Ens de Lyon, CNRS, Centre de Recherche Astrophysique de Lyon UMR5574, F-69230 Saint-Genis-Laval, France

Funder

European Research Council

Federal Ministry of Education and Research

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/2/1689/25430311/sty1958.pdf

Reference55 articles.

1. Astropy: A community Python package for astronomy

2. The MUSE second-generation VLT instrument

3. The effect of stellar rotation on colour-magnitude diagrams: on the apparent presence of multiple populations in intermediate age stellar clusters

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