Add to ORKGA survey of 27 galactic star-forming regions in the 6_K-5_K, 5_K-4_K, and 8_K-7_K CH3CN lines at 110, 92, and 147 GHz, respectively, is made. Twenty-five sources are detected at 110 GHz, nineteen at 92 GHz, and three at 147 GHz. The strongest CH3CN emission arise in hot cores in the regions of massive star formation. CH3CN abundance in these objects is larger than 10^(-9) due to grain mantle evaporation. Weaker CH3CN lines are found in a number of sources. They may arise either in warm (30-50 K) dense (10^(5)-10^(7) cm^(-3)) clouds, or in hot regions accompanied by colder gas
We have studied methyl cyanide, one of the so-called ‘astronomical weeds’, in the 200--277 GHz band....
Context. We perform a laboratory characterization in the 18–1893 GHz range and astronomical detectio...
In recent years the 6.67 GHz masing transition of CH3OH has proven to be a superior tracer of massiv...
The excitation of CH_3CN in the hot core of Orion is examined using high-sensitivity observational d...
We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected mas...
The paper is concerned with the study of the star-forming regions S231–S235 in radio lines of molecu...
$^{a}$ Current address: NASA Goddard Space Flight Center, Earth and Space Data Computing Division, C...
The studies of the complex molecular lines towards the hot molecular cores at millimeter and submill...
Researchers observed CO(7-6), CO(3-2), HCN(3-2) and HCO+(3-2) line emission toward the starburst nuc...
We present the results of a spectral-line survey of the W51e1/e2 star-forming region at 68-88 GHz. 7...
We have used the JCMT to survey molecular line emission towards 14 ultracompact HII regions (G5.89, ...
The studies of the complex molecular emission lines in millimeter and submillimeter wavelengths towa...
We present the initial results of a 3-mm spectral-line survey towards 83 methanol maserselected mass...
We present results of a survey of methyl cyanide (CH3CN) J=12–11 toward 56 sources, including 35 Ext...
Context. We perform a laboratory characterization in the 18–1893 GHz range and astronomical detectio...
We have studied methyl cyanide, one of the so-called ‘astronomical weeds’, in the 200--277 GHz band....
Context. We perform a laboratory characterization in the 18–1893 GHz range and astronomical detectio...
In recent years the 6.67 GHz masing transition of CH3OH has proven to be a superior tracer of massiv...
The excitation of CH_3CN in the hot core of Orion is examined using high-sensitivity observational d...
We present the initial results of a 3-mm spectral-line survey towards 83 methanol maser-selected mas...
The paper is concerned with the study of the star-forming regions S231–S235 in radio lines of molecu...
$^{a}$ Current address: NASA Goddard Space Flight Center, Earth and Space Data Computing Division, C...
The studies of the complex molecular lines towards the hot molecular cores at millimeter and submill...
Researchers observed CO(7-6), CO(3-2), HCN(3-2) and HCO+(3-2) line emission toward the starburst nuc...
We present the results of a spectral-line survey of the W51e1/e2 star-forming region at 68-88 GHz. 7...
We have used the JCMT to survey molecular line emission towards 14 ultracompact HII regions (G5.89, ...
The studies of the complex molecular emission lines in millimeter and submillimeter wavelengths towa...
We present the initial results of a 3-mm spectral-line survey towards 83 methanol maserselected mass...
We present results of a survey of methyl cyanide (CH3CN) J=12–11 toward 56 sources, including 35 Ext...
Context. We perform a laboratory characterization in the 18–1893 GHz range and astronomical detectio...
We have studied methyl cyanide, one of the so-called ‘astronomical weeds’, in the 200--277 GHz band....
Context. We perform a laboratory characterization in the 18–1893 GHz range and astronomical detectio...
In recent years the 6.67 GHz masing transition of CH3OH has proven to be a superior tracer of massiv...