64 citations · 412 across the 24 of their papers we have counts for
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The chemical structure of young high-mass star-forming clumps: (II) parsec-scale CO depletion and deuterium fraction of
S. Feng, D. Li, P. Caselli +19
The physical and chemical properties of cold and dense molecular clouds are key to understanding how stars form. Using the IRAM 30 m and NRO 45 m telescopes, we carried out a Multi…
ALMA Observations of Giant Molecular Clouds in M33. II. Triggered High-mass Star Formation by Multiple Gas Colliding Events at the NGC 604 Complex
Kazuyuki Muraoka, Hiroshi Kondo, Kazuki Tokuda +13
We present the results of ALMA observations in CO(), CO(), and CO() lines and 1.3 mm continuum emission toward a massive ($\sim 10^6 M_{\o…
FRagmentation and Evolution of dense cores Judged by ALMA (FREJA). I (Overview). Inner 1000 au structures of prestellar/protostellar cores in Taurus
Kazuki Tokuda, Kakeru Fujishiro, Kengo Tachihara +11
We have performed survey-type observations in 1 mm continuum and molecular lines toward dense cores (32 prestellar + 7 protostellar) with an average density of 10 cm$^…
A low-velocity bipolar outflow from a deeply embedded object in Taurus revealed by the Atacama Compact Array
Kakeru Fujishiro, Kazuki Tokuda, Kengo Tachihara +11
The first hydrostatic core, the first quasi-hydrostatic object formed during the star formation process, is still the observational missing link between the prestellar and protoste…