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  Near-infrared Emission Lines in Starburst Galaxies at 0.5 < z < 0.9: Discovery of a Merger Sequence of Extreme Obscurations

Calabrò, A., Daddi, E., Cassata, P., Onodera, M., Gobat, R., Puglisi, A., et al. (2018). Near-infrared Emission Lines in Starburst Galaxies at 0.5 < z < 0.9: Discovery of a Merger Sequence of Extreme Obscurations. The Astrophysical Journal, 862.

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Calabrò, A.1, Author
Daddi, E.1, Author
Cassata, P.1, Author
Onodera, M.1, Author
Gobat, R.1, Author
Puglisi, A.1, Author
Jin, S.1, Author
Liu, D.1, Author
Amorín, R.1, Author
Arimoto, N.1, Author
Boquien, M.1, Author
Carraro, R.1, Author
Elbaz, D.1, Author
Ibar, E.1, Author
Juneau, S.1, Author
Mannucci, F.1, Author
Méndez Hernánez, H.1, Author
Oliva, E.1, Author
Rodighiero, G.1, Author
Valentino, F.1, Author
Zanella, A.1, Author more..
Affiliations:
1Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners, ou_2421692              

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Free keywords: dust extinction galaxies: evolution galaxies: high-redshift galaxies: ISM galaxies: starburst infrared: galaxies Astrophysics - Astrophysics of Galaxies Astrophysics - Cosmology and Nongalactic Astrophysics
 Abstract: We obtained optical/near-IR rest-frame Magellan FIRE spectra (including Paβ and Paγ) of 25 starburst galaxies at 0.5 &lt; z &lt; 0.9, with average star formation rates (SFRs) seven times above the main sequence (MS). We find that Paschen-to-Balmer line ratios saturate around a constant value corresponding to A V ̃ 2-3 mag, while line-to-

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 Dates: 2018
 Publication Status: Issued
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Title: The Astrophysical Journal
Source Genre: Journal
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Pages: - Volume / Issue: 862 Sequence Number: - Start / End Page: - Identifier: -