80 citations · 244 across the 4 of their papers we have counts for
9 papers
Millimeter- and Submillimeter-Wave Observations of the OMC-2/3 Region. III. An Extensive Survey for Molecular Outflows
Satoko Takahashi, Masao Saito, Nagayoshi Ohashi +5
Using the ASTE 10 m submillimeter telescope and the 1.4 m Infrared Survey Facility (IRSF), we performed an extensive outflow survey in the Orion Molecular Cloud -2 and -3 region. O…
Millimeter- and Submillimeter-Wave Observations of the OMC-2/3 Region. II. Observational Evidence for Outflow-Triggered Star Formation in the OMC-2 FIR 3/4 Region
Yoshito Shimajiri, Satoko Takahashi, Shigehisa Takakuwa +2
We have carried out the observations of the OMC-2 FIR 3/4 region with the NMA and ASTE in the HCO (1--0), CO (3--2, 1--0), SiO (=0, =2--1), CS (2--1), and…
The CO Molecular Outflows of IRAS 16293-2422 Probed by the Submillimeter Array
Sherry C. C. Yeh, Naomi Hirano, Tyler L. Bourke +4
We have mapped the proto-binary source IRAS 16293-2422 in CO 2-1, 13CO 2-1, and CO 3-2 with the Submillimeter Array (SMA). The maps with resolution of 1".5-5" reveal a single small…
Millimeter- and Submillimeter-Wave Observations of the OMC-2/3 Region; I. Dispersing and Rotating Core around an Intermediate-mass Protostar MMS 7
Satoko Takahashi, Masao Saito, Shigehisa Takakuwa +1
We report the results of H13CO+(1-0), CO(1-0), and 3.3 mm dust continuum observations toward one of the strongest mm-wave sources in OMC-3, MMS 7, with the Nobeyama Millimeter Arra…
Organic Molecules in Low-Mass Protostellar Hot Cores: Submillimeter Imaging of IRAS 16293-2422
Y. -J. Kuan, H. -C. Huang, S. B. Charnley +8
Arcsecond-resolution spectral observations toward the protobinary system IRAS 16293-2422 at 344 and 354 GHz were conducted using the Submillimeter Array. Complex organic molecules…
Submillimeter Array Observations of L1551 IRS 5 in CS (J=7-6)
Shigehisa Takakuwa, Nagayoshi Ohashi, Paul T. P. Ho +7
We have imaged the circumstellar envelope around the binary protostar L1551 IRS 5 in CS (J=7-6) and 343 GHz continuum emission at ~ 3 arcsec resolution using the Submillimeter Arra…