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20162024
most citedTracing Interstellar Heating: An ALCHEMI Measurement of the HCN Isomers in NGC 253

43 citations · 109 across the 7 of their papers we have counts for

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7 papers · 1 filter

astro-ph.GA2024

Synthesis and Spectroscopic Characterization of Interstellar Candidate Ethynyl Thiocyanate: HCCSCN

Elena R. Alonso, Aran Insausti, Lucie Kolesniková +7

This work aims to spectroscopically characterize and provide for the first time direct experimental frequencies of the ground vibrational state and two excited states of the simple…

astro-ph.GA2024

Experimental and computational study of ethanolamine ices at astrochemical conditions

R Ramachandran, Milan Sil, Prasanta Gorai +12

Ethanolamine (NH2CH2CH2OH) has recently been identified in the molecular cloud G+0.693-0.027, situated in the SgrB2 complex in the Galactic center. However, its presence in other r…

astro-ph.GA2022★ 43 cited

Tracing Interstellar Heating: An ALCHEMI Measurement of the HCN Isomers in NGC 253

Erica Behrens, Jeffrey G. Mangum, Jonathan Holdship +17

We analyze HCN and HNC emission in the nearby starburst galaxy NGC 253 to investigate its effectiveness in tracing heating processes associated with star formation. This study uses…

astro-ph.GA2022★ 18 cited

ALCHEMI finds a "shocking" carbon footprint in the starburst galaxy NGC~253

Nanase Harada, Sergio Martin, Jeff Mangum +15

Centers of starburst galaxies may be characterized by a specific gas and ice chemistry due to their gas dynamics and the presence of various ice desorption mechanisms. This may res…

astro-ph.GA2022★ 8 cited

On the thermal structure of the proto-Super Star Cluster 13 in NGC 253

F. Rico-Villas, E. González-Alfonso, J. Martín-Pintado +2

Using high angular resolution ALMA observations ( pc), we study the thermal structure and kinematics of the proto super star cluster in the cen…

astro-ph.GA2022★ 2 cited

Ionise hard: interstellar PO detection

Víctor M. Rivilla, Juan García de la Concepción, Izaskun Jiménez-Serra +13

We report the first detection of the phosphorus monoxide ion (PO) in the interstellar medium. Our unbiased and very sensitive spectral survey towards the G+0.6930.027 mole…