A New Catalog of Globular Clusters in the Milky Way
By W. Harris. 2010
234 citations recorded by the source corpus.
A new revision of the McMaster catalog of Milky Way globular clusters is available. This is the first update since 2003 and the biggest single revision since the original version of the catalog published in 1996. The list now contains a total of 157 objects classified as globular clusters. Major upgrades have been made especially to the cluster coordinates, metallicities, and structural profile parameters, and the list of parameters now also includes central velocity dispersion. NB: This paper is a stand-alone publication available only on the astro-ph archive; it will not be published separately in a journal.
Subfields: Aerospace Engineering, Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/d509e9d791f88c6c8337d64ad69cc1c47158978f
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In Aerospace Engineering
- E. Ricciardelli
- A. Vazdekis
- J. Falc'on-Barroso
- Eugene O. Vasiliev
- M. Koleva
- N. Evans II
- B. Röck
- Sergey E. Koposov
In Astronomy and Astrophysics
- N. Evans II
- V. Belokurov
- Eugene O. Vasiliev
- Sergey E. Koposov
- J. Falc'on-Barroso
- M. Walker
- E. Ricciardelli
- A. Vazdekis
Citations in the corpus
- UV-extended E-MILES stellar population models: young components in massive early-type galaxies (2016, methodology): “To understand whether the HB morphology can have an impact on the integrated colours, we colour-code the clusters according to their HBR parameter (from Harris 2010).”
- The hidden giant: discovery of an enormous Galactic dwarf satellite in Gaia DR2 (2018, background): “9 for references to the MW satellite values used) and black dots show the positions of the MW GCs (Belokurov et al. 2010; Harris 2010; Muñoz et al. 2012; Balbinot et al. 2013; Kim & Jerjen 2015; Kim et al. 2015, 2016a; Laevens et al. 2015; Luque et al. 2016, 2017; Martin et al. 2016a; Weisz et al.…”
- Gaia EDR3 view on galactic globular clusters (2021, background): “Out of 157 objects in the Harris (1996, 2010) catalogue, we could not determine the PM for only a few clusters which are located in highly extincted regions and are not visible to Gaia: 2MASS–GC01, 2MASS–GC02, GLIMPSE01 and GLIMPSE02.”