Discovery of diffuse optical emission lines from the inner Galaxy: Evidence for LI(N)ER-like gas-Reference-Cited by-同舟云学术

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Discovery of diffuse optical emission lines from the inner Galaxy: Evidence for LI(N)ER-like gas

Published:2020-07-03 Issue:27 Volume:6 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

Krishnarao D.¹^ORCID,Benjamin R. A.²^ORCID,Haffner L. M.¹³⁴^ORCID

Affiliation:

1. Department of Astronomy, University of Wisconsin-Madison, 475 N Charter St., Madison, WI 53706, USA.

2. Department of Physics, University of Wisconsin-Whitewater, 800 West Main Street, Whitewater, WI 53190, USA.

3. Department of Physical Sciences, Embry Riddle Aeronautical University, 1 Aerospace Blvd., Daytona Beach, FL 32114, USA.

4. Space Science Institute, 4750 Walnut St., Suite 205, Boulder, CO 80301, USA.

Abstract

Optical emission line observations from the inner Galaxy show that the Milky Way hosts the closest known example of a LI(N)ER.

Funder

National Science Foundation

National Aeronautics and Space Administration

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference60 articles.

1. The Spectra of Some Spiral Nebulae and Globular Star Clusters

2. A relation between distance and radial velocity among extra-galactic nebulae

3. The Apparent Radial Velocities of 100 Extra-Galactic Nebulae

4. A Low-Dispersion UV Glass Spectrograph for the Crossley Reflector

5. Ionized Gas in Spiral and Irregular Galaxies.

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2. Caught in the Act: A Metal-rich High-velocity Cloud in the Inner Galaxy;The Astrophysical Journal;2023-02-01

3. Three-dimensional structure of the central molecular zone;Monthly Notices of the Royal Astronomical Society;2022-08-13

4. Molecular Gas within the Milky Way's Nuclear Wind;The Astrophysical Journal Letters;2021-12-01

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