Publications of the MPIfR Optical & Infrared Interferometry Group


Preibisch, Th. and Zinnecker, H.

Sequentially triggered star formation in OB associations

Triggered Star Formation in a Turbulent ISM
International Astronomical Union. Symposium no. 237
held 14-18 August, 2006 in Prague, Czech Republic,
S237, #47, pg.270-277 (2007)


Abstract
We discuss observational evidence for sequential and triggered star formation in galactic and extragalactic OB associations. We will first review in detail the star formation process in the Scorpius-Centaurus OB association, the nearest OB association to the Sun, where several recent extensive studies have provided comprehensive information on the stellar content and the ages of the different OB subgroups. These data have allowed us to reconstruct the star formation history of the association in some detail and provided important insight into the activity in the rho Oph and Lupus dark clouds, and with the origin of several young stellar groups in the southern sky. After discussing evidence for triggered star formation in and around various other Galactic OB associations (e.g. Ori OB1, Per OB2) we will compare the observational results with recent models of rapid star formation in the turbulent interstellar medium (cf. Briceno et al. chapter in Protostars and Planets V, in press).

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