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View article: Exploring cyanopolyynes towards the C-rich post-AGB star IRAS 22272+5435
Exploring cyanopolyynes towards the C-rich post-AGB star IRAS 22272+5435 Open
Cyanopolyynes are a class of long carbon-chain molecules that are widely distributed in interstellar clouds, but their presence in the circumstellar envelopes (CSEs) of evolved stars appears to be limited to only a few well-studied sources…
View article: The ALMA-QUARKS Survey. III. Clump-to-core Fragmentation and Searches for High-mass Starless Cores
The ALMA-QUARKS Survey. III. Clump-to-core Fragmentation and Searches for High-mass Starless Cores Open
The Querying Underlying mechanisms of massive star formation with ALMA-Resolved gas Kinematics and Structures (QUARKS) survey observed 139 infrared-bright (IR-bright) massive protoclusters at 1.3 mm wavelength with the Atacama Large Millim…
View article: The ALMA-ATOMS survey: A sample of weak hot core candidates identified through line stacking
The ALMA-ATOMS survey: A sample of weak hot core candidates identified through line stacking Open
Context . Hot cores represent critical astrophysical environments for high-mass star formation, distinguished by their rich spectra of organic molecular emission lines. Nevertheless, comprehensive statistical analyses of extensive hot core…
View article: ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – XXI. A large-sample observational study of ethanol and dimethyl ether in hot cores
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions – XXI. A large-sample observational study of ethanol and dimethyl ether in hot cores Open
Hot cores, as a stage of massive star formation, exhibit abundant line emissions of complex organic molecules (COMs). We present a deep line survey of two isomers of C$_2$H$_6$O: ethanol (C$_2$H$_5$OH; EA), and dimethyl ether (CH$_3$OCH$_3…
View article: ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -XXI. A Large-sample Observational Study of Ethanol and Dimethyl Ether in Hot Cores
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -XXI. A Large-sample Observational Study of Ethanol and Dimethyl Ether in Hot Cores Open
Hot cores, as a stage of massive star formation, exhibit abundant line emissions of COMs. We present a deep line survey of two isomers of C$_2$H$_6$O: ethanol (C$_2$H$_5$OH; EA), and dimethyl ether (CH$_3$OCH$_3$; DE) as well as their poss…
View article: The ALMA-ATOMS survey: Vibrationally excited HC<sub>3</sub>N lines in hot cores
The ALMA-ATOMS survey: Vibrationally excited HC<sub>3</sub>N lines in hot cores Open
Context. Interstellar molecules are excellent tools for studying the physical and chemical environments of massive star-forming regions. In particular, the vibrationally excited HC 3 N (HC 3 N*) lines are the key tracers for probing hot co…
View article: The ALMA-ATOMS survey: Vibrationally excited HC$_3$N lines in hot cores
The ALMA-ATOMS survey: Vibrationally excited HC$_3$N lines in hot cores Open
Interstellar molecules are excellent tools for studying the physical and chemical environments of massive star-forming regions. In particular, vibrationally excited HC$_3$N (HC$_3$N*) lines are the key tracers for probing hot cores environ…
View article: Exploring Sulfur Chemistry in TMC-1 with NSRT
Exploring Sulfur Chemistry in TMC-1 with NSRT Open
There have been several studies on sulfur depletion in dense cores like TMC-1 (Taurus Molecular Cloud 1), employing updated reaction networks for sulfur species to explain the missing sulfur in the gas within dense clouds. Most of these st…