All quiet on the Western front? New evidence for massive star formation in Sgr C. Issue Volume 9:Issue S303(2013) (22nd May 2014)

• Record Type: Journal Article
• Authors: Kendrew, Sarah; Ginsburg, Adam; Johnston, Katharine; Beuther, Henrik; Bally, John; Cyganowski, Claudia J.; Battersby, Cara
• Is Part Of: Proceedings of the International Astronomical Union. Volume 9:Issue S303(2013)
• Page Start: 220
• Page End: 222
• Publication Date: 2014-05-22
• Subjects: Astronomy -- Congresses; Astronomy -- Periodicals; 520
• DOI: 10.1017/S174392131400060X
• Languages: English
• ISSNs: 1743-9213

Abstract

Abstract: We summarize here our recent findings from near-infrared spectroscopy and 1 mm line and continuum observations of a recently identified extended green object (EGO) in Sgr C, whose observational characteristics suggest early-stage massive star formation is taking place. Located on the outskirts of the massive evolved Hii region associated with Sgr C in the Western central molecular zone (CMZ), the EGO measures ∼10″ (0.4 pc at 8.5 kpc). We confirm that early-stage star formation is taking place on the periphery of the Sgr C Hii region. The data show clear detections of two protostellar cores and several knots of H2 and Brackett γ emission alongside a previously detected compact radio source. We calculate the cores' joint mass to be ∼10 3 M⊙, with column densities of 1-2 × 10 24 cm −2 . The host molecular clouds mass is approximately 10 5 M⊙ . Despite these favorable conditions, the cloud is curiously devoid of any further star formation, making it comparable to other remarkably quiescent clouds, such as G0.253 in the Eastern CMZ.