Kinematic evidence for feedback-driven star formation in NGC 1893. Issue 2 (17th March 2018)

• Record Type: Journal Article
• Authors: Lim, Beomdu; Sung, Hwankyung; Bessell, Michael S; Lee, Sangwoo; Lee, Jae Joon; Oh, Heeyoung; Hwang, Narae; Park, Byeong-Gon; Hur, Hyeonoh; Hong, Kyeongsoo; Park, Sunkyung
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 477:Issue 2(2018)
• Page Start: 1993
• Page End: 2003
• Publication Date: 2018-03-17
• Subjects: stars: formation -- stars: kinematics and dynamics -- H ii regions -- ISM: kinematics and dynamics -- open clusters and associations: individual (NGC 1893); Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/sty713
• Languages: English
• ISSNs: 0035-8711

Abstract

Abstract: OB associations are the prevailing star-forming sites in the Galaxy. Up to now, the process of how OB associations were formed remained a mystery. A possible process is self-regulating star formation driven by feedback from massive stars. However, although a number of observational studies uncovered various signposts of feedback-driven star formation, the effectiveness of such feedback has been questioned. Stellar and gas kinematics is a promising tool to capture the relative motion of newborn stars and gas away from ionizing sources. We present high-resolution spectroscopy of stars and gas in the young open cluster NGC 1893. Our findings show that newborn stars and the tadpole nebula Sim 130 are moving away from the central cluster containing two O-type stars, and that the time-scale of sequential star formation is about 1 Myr within a 9 pc distance. The newborn stars formed by feedback from massive stars account for at least 18 per cent of the total stellar population in the cluster, suggesting that this process can play an important role in the formation of OB associations. These results support the self-regulating star formation model.