S. Ragan

activity

20232025

^{13}

J = 3 \to 2

emission in the Central Molecular Zone

2 citations · 2 across the 6 of their papers we have counts for

collaborators

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astro-ph.GA2024★ 2 cited

CHIMPS2: $^{13}$ CO $J = 3 \to 2$ emission in the Central Molecular Zone

S. M. King, T. J. T. Moore, J. D. Henshaw +12

We present the initial data for the ( $J = 3 \to 2$ ) transition of $^{13}$ CO obtained from the Central Molecular Zone (CMZ) of the Milky Way as part of the CO Heterodyne Inner Milky…

astro-ph.GA2024

NEATH III: a molecular line survey of a simulated star-forming cloud

F. D. Priestley, P. C. Clark, S. C. O. Glover +4

We present synthetic line observations of a simulated molecular cloud, utilising a self-consistent treatment of the dynamics and time-dependent chemical evolution. We investigate l…

astro-ph.GA2024

N $_{2}$ H $^{+}$ (1-0) as a tracer of dense gas in and between spiral arms

O. Feher, S. E. Ragan, F. D. Priestley +2

Recent advances in identifying giant molecular filaments in galactic surveys allow us to study the interstellar material and its dense, potentially star forming phase on scales com…

CHIMPS2: 13CO J=3→2 emission in the Central Molecular Zone

NEATH III: a molecular line survey of a simulated star-forming cloud

N2​H+(1-0) as a tracer of dense gas in and between spiral arms

CHIMPS2: $^{13}$ CO $J = 3 \to 2$ emission in the Central Molecular Zone

N $_{2}$ H $^{+}$ (1-0) as a tracer of dense gas in and between spiral arms