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Ices regulate much of the chemistry during star formation and account for up to 80% of the available oxygen and carbon. In this paper, we use the Spitzer c2d ice survey, complimented with data sets on...
Gas-phase complex organic molecules are commonly detected toward high-mass protostellar hot cores. Detections toward low-mass protostars and outflows are comparatively rare, and a larger sample is key...
We report on simulations of the formation of the first stars in the Universe, where we identify regions of hot atomic gas (fH2 < 10-6) at densities above 10-14 g/cc, heated to temperatures ranging bet...
Spectral observations of molecular line profiles reveal the so-called ‘blue profiles’ for double-peaked molecular lines with stronger blue and weaker red peaks as notable features for star-forming cl...
We explore the origin of a population of distant companions (~1000 - 5000 AU) to Class I protostellar sources recently found by Connelley and co-workers, who noted that the companion fraction diminish...
We present new observations of near-infrared molecular hydrogen (H2) line emission in a sample of 18 Class I and flat-spectrum low mass protostars, primarily in the Tau- Aur and {\rho} Oph dark clouds...
Multiple protostars, jets, and the origin of brown Dwarfs。
The Spin History of Protostars:Disk Locking, Revisited。
From dust to gas ... and the infrared to the millimetric: Doubly deuterated molecules in protostars

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