We investigate the warm ionized gas in the blue compact galaxy (BCG) Haro 14 by means of integral field spectroscopic observations taken with the Multi Unit Spectroscopic Explorer (MUSE) at the Very Large Telescope. The large field of view of MUSE and its unprecedented sensitivity enable observations of the galaxy nebular emission up to large galactocentric distances, even in the important but very faint [O
International audienceWe have used the Multi-Unit Spectroscopic Explorer (MUSE) to study the circumg...
We report the identification of extended Ly alpha nebulae at z similar or equal to 3.3 in the Hubble...
International audienceThe origin of the cold gas in central galaxies in groups is still a matter of ...
We investigate the warm ionized gas in the blue compact galaxy (BCG) Haro 14 by means of integral fi...
We investigate the warm ionized gas in the blue compact galaxy (BCG) Haro 14 by means of integral fi...
Context. Low-luminosity, gas-rich blue compact galaxies (BCG) are ideal laboratories to investigate ...
Investigations of blue compact galaxies (BCGs) are essential to advancing our understanding of galax...
Investigations of blue compact galaxies (BCGs) are essential to advancing our understanding of galax...
Gas in the circumgalactic medium can be probed to low column densities using sightlines towards brig...
<p>I will present the most up-to-date observations of ionisation, excitation and absorption lines in...
There can be no complete discussion of the ``cosmic noon" epoch and early galaxy formation without r...
We report the identification of extended Lyα nebulae at z ≃ 3.3 in the Hubble Ultra Deep Field (HUDF...
We report the identification of extended Ly\u3b1 nebulae at z 43 3.3 in the Hubble Ultra Deep Field...
19 pages, 12 figures, accepted for publication in MNRASInternational audienceWe report new wide-fiel...
Context. Blue compact galaxies (BCG) are gas-rich, low-mass, small systems that form stars at unusua...
International audienceWe have used the Multi-Unit Spectroscopic Explorer (MUSE) to study the circumg...
We report the identification of extended Ly alpha nebulae at z similar or equal to 3.3 in the Hubble...
International audienceThe origin of the cold gas in central galaxies in groups is still a matter of ...
We investigate the warm ionized gas in the blue compact galaxy (BCG) Haro 14 by means of integral fi...
We investigate the warm ionized gas in the blue compact galaxy (BCG) Haro 14 by means of integral fi...
Context. Low-luminosity, gas-rich blue compact galaxies (BCG) are ideal laboratories to investigate ...
Investigations of blue compact galaxies (BCGs) are essential to advancing our understanding of galax...
Investigations of blue compact galaxies (BCGs) are essential to advancing our understanding of galax...
Gas in the circumgalactic medium can be probed to low column densities using sightlines towards brig...
<p>I will present the most up-to-date observations of ionisation, excitation and absorption lines in...
There can be no complete discussion of the ``cosmic noon" epoch and early galaxy formation without r...
We report the identification of extended Lyα nebulae at z ≃ 3.3 in the Hubble Ultra Deep Field (HUDF...
We report the identification of extended Ly\u3b1 nebulae at z 43 3.3 in the Hubble Ultra Deep Field...
19 pages, 12 figures, accepted for publication in MNRASInternational audienceWe report new wide-fiel...
Context. Blue compact galaxies (BCG) are gas-rich, low-mass, small systems that form stars at unusua...
International audienceWe have used the Multi-Unit Spectroscopic Explorer (MUSE) to study the circumg...
We report the identification of extended Ly alpha nebulae at z similar or equal to 3.3 in the Hubble...
International audienceThe origin of the cold gas in central galaxies in groups is still a matter of ...