Unveiling Kinematic Structure in the Starburst Heart of NGC 253

Monthly Notices of the Royal Astronomical Society(2020)

Cited 3|Views11
No score
Abstract
We observed the Brackett α emission line (4.05 μm) within the nuclear starburst of NGC 253 to measure the kinematics of ionized gas, and distinguish motions driven by star formation feedback from gravitational motions induced by the central mass structure. Using NIRSPEC on Keck II, we obtained 30 spectra through a $0^{\prime \prime }_{.}5$ slit stepped across the central ∼5 arcsec × 25 arcsec (85 ...
More
Translated text
Key words
galaxies: individual: NGC 253,galaxies: kinematics and dynamics,galaxies: nuclei,galaxies: starburst,galaxies: ISM
AI Read Science
Must-Reading Tree
Example
Generate MRT to find the research sequence of this paper
Chat Paper
Summary is being generated by the instructions you defined