Spectra and radial velocities of nuclear stars Virtual Observatory Resource

Authors

1. Feldmeier A.
2. Neumayer N.
3. Seth A.
4. Schodel R.
5. Lutzgendorf N.,de Zeeuw P.T.
6. Kissler-Patig M.
7. Nishiyama S.
8. Walcher C.J.

Published by

CDS

Abstract

Within the central 10pc of our Galaxy lies a dense cluster of stars. This nuclear star cluster forms a distinct component of the Galaxy, and similar nuclear star clusters are found in most nearby spiral and elliptical galaxies. Studying the structure and kinematics of nuclear star clusters reveals the history of mass accretion and growth of galaxy nuclei and central massive black holes. Because the Milky Way nuclear star cluster is at a distance of only 8 kpc, we can spatially resolve the cluster on sub-parsec scales. This makes the Milky Way nuclear star cluster a reference object for understanding the formation of all nuclear star clusters.

Keywords

1. radial-velocity
2. infrared-astronomy
3. spectroscopy

Bibliographic source Bibcode

2014A&A...570A...2F

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/570/A2

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/570/A2

Document Object Identifer DOI

doi:10.26093/cds/vizier.35700002

Access

Web browser access HTML

https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/570/A2
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/570/A2
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/570/A2

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IVOA Cone Search SCS

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https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/570/A2/mw_star?
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