Studying the ISM at ∼10 pc scale in NGC 7793 with MUSE. I. Data description and properties of the ionised gas

Lorenza Della Bruna,Angela Adamo,Arjan Bik,Michele Fumagalli,Rene A. M. Walterbos,Göran Östlin,Gustavo Bruzual,Daniela Calzetti,Stephane Charlot,Kathryn Grasha,Linda J. Smith,David Thilker,Aida Wofford

Studying the ISM at ∼10 pc scale in NGC 7793 with MUSE. I. Data description and properties of the ionised gas

2020

Lorenza Della Bruna
Angela Adamo
Arjan Bik
Michele Fumagalli
Rene A. M. Walterbos
Göran Östlin
Gustavo Bruzual
Daniela Calzetti
Stephane Charlot
Kathryn Grasha
Linda J. Smith
David Thilker
Aida Wofford

Context. Studies of nearby galaxies reveal that around 50% of the total H alpha luminosity in late-type spirals originates from diffuse ionised gas (DIG), which is a warm, diffuse component of the ...

Keywords:

Galaxy
Physics
H-alpha
Astrophysics
data description
Luminosity

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