Outlying Hα emitters in SDSS IV MaNGA
Author:
Affiliation:
1. National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Post Bag 3, Ganeshkhind, Pune 411 007, India
2. Indian Institute of Astrophysics (IIA), II Block, Koramangala, Bengaluru 560 034, India
Funder
National Science Foundation
U.S. Department of Energy
Science and Technology Facilities Council
National Aeronautics and Space Administration
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/485/1/428/27940391/stz433.pdf
Reference46 articles.
1. The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the Extended Baryon Oscillation Spectroscopic Survey and from the Second Phase of the Apache Point Observatory Galactic Evolution Experiment
2. Classification parameters for the emission-line spectra of extragalactic objects
3. SDSS IV MaNGA – spatially resolved diagnostic diagrams: a proof that many galaxies are LIERs
4. Large-scale bipolar wind in M82
5. The SAMI Galaxy Survey: instrument specification and target selection
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3. A Giant Shell of Ionized Gas Discovered near M82 with the Dragonfly Spectral Line Mapper Pathfinder;The Astrophysical Journal;2022-03-01
4. SDSS-IV MaNGA: the physical origin of off-galaxy H α blobs in the local Universe;Monthly Notices of the Royal Astronomical Society;2021-10-02
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