GMOS–IFU spectroscopy of the compact H iigalaxies Tol 0104−388 and Tol 2146−391: the dependence on the properties of the interstellar medium

Author:

Lagos P.1,Telles E.2,Nigoche-Netro A.3,Carrasco E. R.4

Affiliation:

1. Centro de Astrofísica da Universidade do Porto; Rua das Estrelas; 4150-762; Porto; Portugal

2. Observatório Nacional; Rua José Cristino, 77; Rio de Janeiro; 20921-400; Brazil

3. Instituto de Astronomía y Meteorología; Av, Vallarta 2602. Col. Arcos Vallarta, Guadalajara; Jalisco; CP; 44130; Mexico

4. Gemini Observatory/AURA; Southern Operations Center; Casilla 603; La Serena; Chile

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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2. Spatially resolved properties of the ionized gas in the H ii galaxy J084220+115000;Monthly Notices of the Royal Astronomical Society;2023-01-09

3. Warm ionized gas in the blue compact galaxy Haro 14 viewed by MUSE;Astronomy & Astrophysics;2022-08

4. Inverted metallicity gradients in two Virgo cluster star-forming dwarf galaxies: evidence of recent merging?;Monthly Notices of the Royal Astronomical Society;2020-08-31

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