PG
Prasanta Gorai
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Astro and Planetary Science
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Publications (163)
- A Cyanopolyyne-rich but Complex-organic-molecule-poor Massive Protostar: The First Hot Carbon-chain Chemistry Source G28.28-0.36 Save
- SOMA: The SOFIA Massive Radio Survey. III. Radio Emission from Intermediate-mass Protostars Save
- ALMA reveals an explosive outflow candidate in IRAS 16119−5048 Save
- Nondetection of HC(S)SH: Estimating Upper Limits and Constraining Chemistry* Save
- A surprisingly large asymmetric ejection from Mira A Save
- Binding energy distributions of alcohols, thiols, and their precursors on interstellar water ice surfaces Save
- Chemical complexity in star formation induced by stellar feedback: Cores shock-formed by the supernova remnant W44 Save
- ALMA Observations of Cold Methanol Gas in the Large Magellanic Cloud: N79 South Giant Molecular Cloud Save
- The SOFIA Massive (SOMA) Radio Survey. II. Radio Emission from High-luminosity Protostars Save
- A surprisingly large asymmetric ejection from Mira A Save
- ALMA Reveals an Explosive Outflow Candidate in IRAS 16119–5048 Save
- ALMA-QUARKS View of W49N: Multipolar Episodic Outflow Associated with the Most Energetic Galactic Water Maser Save
- ALMA-QUARKS view of W49N: Multipolar episodic outflow associated with the most energetic Galactic water maser Save
- An eccentric massive protobinary assembled via a core merger parabolic encounter Save
- An eccentric massive protobinary assembled via a core-merger parabolic encounter Save
- Complex organic molecules and cosmic ray ionisation rate towards the massive protostar Cepheus A HW2 Save
- Evolution of Starless Cores in Massive Clumps Seen by the ALMA ASHES and QUARKS Surveys Save
- Evolution of starless cores in massive clumps seen by the ALMA ASHES and QUARKS surveys Save
- Herschel/HIFI Observations of Molecular Lines Toward G10.47+0.03 Save
- Herschel/HIFI observations of molecular lines toward G10.47+0.03 Save