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1887
4179802
The small sizes and high implied densities of ``Little Red Dots'' with Balmer Breaks could explain their broad emission lines without an Active Galactic Nucleus
Author(s):
Baggen, J.F.W.; Dokkum, P. van; Brammer, G.; Graaff, A.G. de; Franx, M. (
0000-0002-8871-3026
); Greene, J.; Labbé, I.; Leja, J.; Maseda, M.V.; Nelson, E.J.; Rix, H.-W.; Wang, B.; Weibel, A.
Published
2024
Publication type
Article / Letter to editor
Date issued
2024
Language
English
Is part of
Astrophysical Journal Letters (2024), No. 1, L13
hdl
1887/4179802
doi
10.3847/2041-8213/ad90b8
URL
https://ui.adsabs.harvard.edu/abs/2024ApJ...977L..13B
Persistent identifier url
https://hdl.handle.net/1887/4179802
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