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HIGH-RESOLUTION SUBMILLIMETER MULTILINE OBSERVATIONS OF G19.61−0.23: SMALL-SCALE CHEMISTRY
We present the Submillimeter Array (SMA) observations of molecular lines at 330 and 340?GHz toward G19.61 ? 0.23. The SMA observations have a spatial resolution of ~2'' and a bandpass of 2?? 2?GHzExpand
Massive molecular outflows associated with UCHII/HII regions
Received date ; Accepted date Abstract. Aims: We searched for the molecular outflows from fifteen mole cular clouds associated with ultra-compact and compact HII (UCHII/HII) regions and discussedExpand
A systemic study of 14 southern infrared dark clouds with N2H+, HNC, HCO+ and HCN lines
We have studied 14 southern infrared dark clouds (IRDCs) using the data taken from the Millimetre Astronomy Legacy Team 90 GHz (MALT90) survey and the GLIMPSE and MIPSGAL mid-infrared survey of theExpand
STAR FORMATION ASSOCIATED WITH THE SUPERNOVA REMNANT IC443
We have performed submillimeter and millimeter observations in CO lines toward supernova remnant (SNR) IC443. The CO molecular shell coincides well with the partial shell of the SNR detected in radioExpand
Gas Kinematics and Star Formation in the Filamentary IRDC G34.43+0.24
We performed a multiwavelength study toward infrared dark cloud (IRDC) G34.43+0.24. New maps of 13CO $J$=1-0 and C18}O J=1-0 were obtained from the Purple Mountain Observatory (PMO) 13.7 m radioExpand
Physical properties, kinematics and mass function of 12 northern infrared dark clouds
The physical, chemical and kinetic characteristics of 12 northern infrared dark clouds (IRDCs) are systematic studied using the $\rm ^{13}CO $ (1-0) and $\rm C^{18}O$ (1-0) lines, observed with theExpand
A molecular line study towards massive extended green object clumps in the southern sky: chemical properties
We present a molecular line study towards 31 extended green object (EGO) clumps in the southern sky using data from MALT90 (Millimetre Astronomy Legacy Team 90 GHz). According to previousExpand
The open cluster NGC 6823 and possible triggered star formation associated with SNR G59.5+0.1
Aims. We investigate the environment in the vicinity of the supernova remnant (SNR) G59.5+0.1 and identify all the young stellar objects (YSOs) around the SNR, to derive the physical properties,Expand
OH Survey along Sightlines of Galactic Observations of Terahertz C
We have obtained OH spectra of four transitions in the $^2\Pi_{3/2}$ ground state, at 1612, 1665, 1667, and 1720 MHz, toward 51 sightlines that were observed in the Herschel project GalacticExpand
Infall and Outflow of Molecular Gas in Sgr B2
Observations of two H2CO (303-202 and 321-220) lines and continuum emission at 1.3 mm toward Sgr B2(N) and Sgr B2(M) have been carried out with the SMA. The mosaic maps of Sgr B2(N) and Sgr B2(M) inExpand
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