Deep photometric studies in the Third Quadrant: NGC 2467

Details Deep photometric studies in the Third Quadrant: NGC 2467 Deep photometric studies in the Third Quadrant: NGC 2467

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26...72g&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

2

Galaxy: Structure, Open Clusters And Associations: Individual: Haffner 18, Haffner 19, Ngc 2467

Scientific paper

The region of NGC 2467, placed in the ``Puppis Window'' of the third quadrant, contains a number of young open clusters and nebular entities reported at different distances. We present a new analysis of the field of NGC 2467 based on deep images, in the UBVRI filters, obtained with the 2.2-m MPG/ESO telescope at La Silla Observatory, Chile. We analyze the stellar content and establish new distances to the clusters. We suggest the presence of a population of young stellar objects, including the detection of HH-like features. Also, we discover tens of background galaxies seen through the galactic plane.

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