Evidences of enhanced formation episodes in the Galactic open cluster system

PIATTI, ANDRÉS E.

ASTRONOMY AND ASTROPHYSICS

EDP SCIENCES S A

Año: 2010 vol. 513 p. 1 - 4

0004-6361

The exciting debate about the existence of signs of enhanced formation of Galactic open clusters (OCs) is revisited here on the basis of a revised age distribution.} {The data were taken from the recently updated 2009 version of the Dias et al.´s 1787 OC catalogue.} { We found that the present OC´s age distribution presents two primary  excesses at $t$ $sim$ 10-15 Myr and 1.5 Gyr, which are signs of enhanced formation episodes similar  to those that occurred in other galaxies (e.g., M,51, NGC,1705).  When restricting the OC sample to those located in the solar neighbourhood,  with the aim of avoiding incompleteness  effects,  we also find  that these clusters are engraved with clear signs of enhanced formation at both ages.