THE DEUTERIUM FRACTION IN MASSIVE STARLESS CORES AND DYNAMICAL IMPLICATIONS

• Published in: The Astrophysical journal Vol. 821; no. 2; p. 94
• Main Authors: Kong, Shuo, Tan, Jonathan C., Caselli, Paola, Fontani, Francesco, Pillai, Thushara, J. Butler, Michael, Shimajiri, Yoshito, Nakamura, Fumitaka, Sakai, Takeshi
• Format: Journal Article
• Language: English
• Published: The American Astronomical Society 20.04.2016
• Subjects: Clouds; Collapse; Deuteration; Deuterium; Estimates; evolution; Fittings; Fractionation; ISM: clouds; ISM: magnetic fields; ISM: structure; stars: formation; Texts
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/0004-637X/821/2/94

ABSTRACT We study deuterium fractionation in two massive starless/early-stage cores, C1-N and C1-S, in Infrared Dark Cloud G028.37+00.07, which was first identified by Tan et al. with ALMA. Line emission from multiple transitions of N2H+ and N2D+ were observed with the ALMA, CARMA, SMA, JCMT, NRO 45 m, and IRAM 30 m telescopes. By simultaneously fitting the spectra, we estimate the excitation conditions and deuterium fraction, D frac N 2 H + [ N 2 D + ] / [ N 2 H + ] , with values of D frac N 2 H + 0.2-0.7, several orders of magnitude above the cosmic [D]/[H] ratio. Additional observations of o-H2D+ are also presented that help constrain the ortho-to-para ratio of H2, which is a key quantity affecting the degree of deuteration. We then present chemodynamical modeling of the two cores, especially exploring the implications for the collapse rate relative to free-fall, ff. In order to reach the high level of observed deuteration of N 2 H + , we find that the most likely evolutionary history of the cores involves collapse at a relatively slow rate, one-tenth of free-fall.