activity
20072023
most citedSpatial correlation between submillimetre and Lyman-alpha galaxies in the SSA 22 protocluster

110 citations · 762 across the 29 of their papers we have counts for

collaborators

29 papers

astro-ph.GA2023

Distributions of the Density and Kinetic Temperature of the Molecular Gas in the Central Region of NGC 613 using Hierarchical Bayesian Inference

Hiroyuki Kaneko, Tomoka Tosaki, Kunihiko Tanaka +1

We present position-position-velocity (PPV) cubes of the physical and chemical properties of the molecular medium in the central 1.2 kpc region of the active galaxy NGC 613 at a PP…

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★ 32 cited

Energizing Star Formation: The Cosmic Ray Ionization Rate in NGC 253 Derived From ALCHEMI Measurements of HO and SO

Jonathan Holdship, Jeffrey G. Mangum, Serena Viti +16

The cosmic ray ionization rate (CRIR) is a key parameter in understanding the physical and chemical processes in the interstellar medium. Cosmic rays are a significant source of en…

astro-ph.GA2021★ 34 cited

Starburst Energy Feedback Seen Through HCO/HOC Emission in NGC 253 from ALCHEMI

Nanase Harada, Sergio Martín, Jeffrey G. Mangum +19

Molecular abundances are sensitive to UV-photon flux and cosmic-ray ionization rate. In starburst environments, the effects of high-energy photons and particles are expected to be…

astro-ph.GA2021★ 6 cited

Atomic Carbon in the Central Molecular Zone of the Milky Way : Possible Cosmic-ray Induced Chemistry or Time-Dependent Chemistry Associated with SNR Sagittarius A East

Kunihiko Tanaka, Makoto Nagai, Kazuhisa Kamegai

Being one of the most abundant atomic/molecular species observed in dense molecular gas, atomic carbon () is a potential good tracer of molecular gas mass in many che…