most citedInterstellar detection of O-protonated carbonyl sulfide, HOCS+

1 citations · 1 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2024

Double, double, toil, and trouble: The tails, bubbles, and knots of the local compact obscured nucleus galaxy NGC4418

C. F. Wethers, S. Aalto, G. C. Privon +20

Compact obscured nuclei (CONs) are an extremely obscured (N >10 cm) class of galaxy nuclei thought to exist in 20-40 per cent of nearby (ultra-)luminous infrar…

astro-ph.GA20241 cited

Interstellar detection of O-protonated carbonyl sulfide, HOCS+

Miguel Sanz-Novo, Víctor M. Rivilla, Izaskun Jiménez-Serra +12

We present the first detection in space of O-protonated carbonyl sulfide (\ch{HOCS+}), in the midst of an ultradeep molecular line survey toward the G+0.693-0.027 molecular cloud.…

astro-ph.GA2024

Molecular isotopologue measurements toward super star clusters and the relation to their ages in NGC253 with ALCHEMI

J. Butterworth, S. Viti, P. P. Van der Werf +18

Determining the evolution of the CNO isotopes in the interstellar medium (ISM) of starburst galaxies can yield important constraints on the ages of superstar clusters (SSCs), or on…

astro-ph.GA2024

CON-quest II. Spatially and spectrally resolved HCN/HCO+ line ratios in local luminous and ultraluminous infrared galaxies

Y. Nishimura, S. Aalto, M. D. Gorski +24

Nuclear regions of ultraluminous and luminous infrared galaxies (U/LIRGs) are powered by starbursts and/or active galactic nuclei (AGNs). These regions are often obscured by extrem…

astro-ph.GA2024

The ALCHEMI atlas: principal component analysis reveals starburst evolution in NGC 253

Nanase Harada, David S. Meier, Sergio Martín +24

Molecular lines are powerful diagnostics of the physical and chemical properties of the interstellar medium (ISM). These ISM properties, which affect future star formation, are exp…