2MASS NIR photometry for 693 candidate globular clusters in M 31 and the Revised Bologna Catalogue
By S. Galleti, L. Federici, M. Bellazzini, F. F. Pecci, S. Macrina. 2003
175 citations recorded by the source corpus.
We have identified in the 2MASS database 693 known and candidate globular clusters in M 31. The 2MASS J, H, K magnitudes of these objects have been transformed to the same homogeneous photometric system of existing near infrared photometry of M 31 globulars, finally yielding J, H, K integrated photometry for 279 confirmed M 31 clusters, 406 unconfirmed candidates and 8 objects with controversial classification. Of these objects 529 lacked any previous estimate of their near infrared magnitudes. The newly assembled near infrared dataset has been implemented into a revised version of the Bologna Catalogue of M 31 globulars, with updated optical (UBVRI) photometry taken, when possible, from the most recent sources of CCD photometry available in the literature and transformed to a common photometric system. The final Revised Bologna Catalogue (available in electronic form) is the most comprehensive list presently available of confirmed and candidate M 31 globular clusters, with a total of 1164 entries. In particular, it includes 337 confirmed GCs, 688 GC candidates, 10 objects with controversial classification, 70 confirmed galaxies, 55 confirmed stars, and 4 H regions lying within ∼3 ◦ from the center of the M 31 galaxy. Using the newly assembled database we show that the V − K color provides a powerful tool to discriminate between M 31 clusters and background galaxies, and we identify a sample of 83 globular cluster candidates, which is not likely to be contaminated by misclassified galaxies.
Subfields: Astronomy and Astrophysics, Instrumentation
View Paper: https://www.semanticscholar.org/paper/59c8c5a4f66a181d869efbfdb3537bbca1007058
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Citations in the corpus
- The Detailed Star Formation History in the Spheroid, Outer Disk, and Tidal Stream of the Andromeda Galaxy (2006, background): “In the subsequent observations of the tidal stream and outer disk, there was only a candidate globular cluster (Bol D242; Galleti et al. 2004) nearour optimal position in the stream, and no known globular clusters near our optimal position in the disk.”
- Galactic stellar haloes in the CDM model (2009, unknown): “5, 2008 March; Galleti et al. 2004, 2006, 2007; Kim et al. 2007; Huxor et al. 2008).”
- Stars beyond galaxies: the origin of extended luminous haloes around galaxies (2005, unknown): “…caveat of small number statistics (only∼ 150 globular clusters around the Galaxy and ∼ 360 around M31 are currently confirmed; see Harris 1996 and [t] Galleti et al 2004), it is interesting that a Sersic law withn ∼ 6 is consistent with the (projected) number density profile of Galactic globulars.”