Add to ORKGOriginal paper can be found at http://www.astrosociety.org/pubs/cs/156-194.html--Copyright Astronomical Society of the PacificIs atomic hydrogen a precursor to or byproduct of the star formation process? Recent evidence suggests that a large percentage of the atomic hydrogen in spiral galaxies could be due to photodissociation of molecular gas by UV radiation from hot young stars
In this Letter, we present for the first time images and kinematics of neutral hydrogen, which is un...
[[abstract]]It has long been recognized that interactions between galaxies are important in determin...
We study the atomic (H i) and molecular hydrogen (H2) contents of early-type galaxies (ETGs) and the...
Hydrogen is thought to be the most common 'ordinary' matter in the universe. It can combine to form ...
none11si©: 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomic...
Young massive stars produce Far-UV photons which dissociate the molecular gas on the surfaces of the...
The current cosmological model, the Lambda CDM theory, describes with remarkable precision the assem...
Context. Despite many studies of star formation in spiral galaxies, a complete and coherent understa...
The VATLY radio telescope has been used to draw the map of atomic hydrogen gas in the disk of the Mi...
© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
The extended, fragile, collisional atomic hydrogen (HI) gas discs in galaxies are excellent diagnost...
International audienceLong gamma-ray bursts (GRBs), among the most energetic events in the Universe,...
Shocked molecular hydrogen has been observed around the nucleus of the nearby galaxy, NGC 253. This ...
It has long been recognized that interactions between galaxies are important in determining their ev...
IT has long been recognized that interactions between galaxies are important in determining their ev...
In this Letter, we present for the first time images and kinematics of neutral hydrogen, which is un...
[[abstract]]It has long been recognized that interactions between galaxies are important in determin...
We study the atomic (H i) and molecular hydrogen (H2) contents of early-type galaxies (ETGs) and the...
Hydrogen is thought to be the most common 'ordinary' matter in the universe. It can combine to form ...
none11si©: 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomic...
Young massive stars produce Far-UV photons which dissociate the molecular gas on the surfaces of the...
The current cosmological model, the Lambda CDM theory, describes with remarkable precision the assem...
Context. Despite many studies of star formation in spiral galaxies, a complete and coherent understa...
The VATLY radio telescope has been used to draw the map of atomic hydrogen gas in the disk of the Mi...
© 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Societ...
The extended, fragile, collisional atomic hydrogen (HI) gas discs in galaxies are excellent diagnost...
International audienceLong gamma-ray bursts (GRBs), among the most energetic events in the Universe,...
Shocked molecular hydrogen has been observed around the nucleus of the nearby galaxy, NGC 253. This ...
It has long been recognized that interactions between galaxies are important in determining their ev...
IT has long been recognized that interactions between galaxies are important in determining their ev...
In this Letter, we present for the first time images and kinematics of neutral hydrogen, which is un...
[[abstract]]It has long been recognized that interactions between galaxies are important in determin...
We study the atomic (H i) and molecular hydrogen (H2) contents of early-type galaxies (ETGs) and the...