We present new optical and radio spectroscopic observations of the remarkable galaxy Malin 1. This galaxy has unique features that include an extremely low surface brightness disk with an enormous mass of neutral hydrogen, and a low luminosity Seyfert nucleus. Malin 1 is exceptional in its values of MHO, LB, and MHI /Ln, and modest in its surface mass density of gas and stars. Spirals with large Min /LB tend to have low mean column densities of HI, and are close to the threshold for star formation due to instabilities in a rotating gas disk. In these terms, Malin 1 has a disk with extremely inefficient star formation. The bulge spectrum is dominated by the absorption features of an old, metal rich stellar population, although there is some ...
We present Megacam deep optical images (g and r) of Malin 1 obtained with the 6.5m Magellan/Clay tel...
Our R-band data show that the optical light from Malin 1 corresponds well with the >2-arcmin extent ...
none16siThis article has been accepted for publication in MNRAS Letters ©: 2018 The Author(s) Publis...
International audienceContext. Malin 1 is the largest known low surface brightness (LSB) galaxy, the...
A study of the Galactic Center stellar population is continuing with a sensitive 2μm CCD camera. Usi...
Context. Low surface brightness galaxies (LSBGs) represent a significant percentage of local galaxie...
International audienceContext. Low surface brightness galaxies (LSBGs) represent a significant perce...
International audienceLow Surface Brightness galaxies (LSBs) represent a significant fraction of gal...
Since its discovery, Malin 1 has been considered the prototype and most extreme example of the class...
Giant low-surface brightness (GLSB) galaxies are an extreme class of objects with very faint and ext...
The low surface brightness disc galaxy Malin 2 challenges the “standard ” theory of galaxy evolution...
Context. Low surface brightness galaxies (LSBGs) represent a significant percentage of local galaxie...
Malin 1 has long been considered a prototype giant, dark matter dominated Low Surface Brightness gal...
Malin 1 has long been considered a prototype giant, dark matter dominated Low Surface Brightness gal...
We present Megacam deep optical images (g and r) of Malin 1 obtained with the 6.5m Magellan/Clay tel...
Our R-band data show that the optical light from Malin 1 corresponds well with the >2-arcmin extent ...
none16siThis article has been accepted for publication in MNRAS Letters ©: 2018 The Author(s) Publis...
International audienceContext. Malin 1 is the largest known low surface brightness (LSB) galaxy, the...
A study of the Galactic Center stellar population is continuing with a sensitive 2μm CCD camera. Usi...
Context. Low surface brightness galaxies (LSBGs) represent a significant percentage of local galaxie...
International audienceContext. Low surface brightness galaxies (LSBGs) represent a significant perce...
International audienceLow Surface Brightness galaxies (LSBs) represent a significant fraction of gal...
Since its discovery, Malin 1 has been considered the prototype and most extreme example of the class...
Giant low-surface brightness (GLSB) galaxies are an extreme class of objects with very faint and ext...
The low surface brightness disc galaxy Malin 2 challenges the “standard ” theory of galaxy evolution...
Context. Low surface brightness galaxies (LSBGs) represent a significant percentage of local galaxie...
Malin 1 has long been considered a prototype giant, dark matter dominated Low Surface Brightness gal...
Malin 1 has long been considered a prototype giant, dark matter dominated Low Surface Brightness gal...
We present Megacam deep optical images (g and r) of Malin 1 obtained with the 6.5m Magellan/Clay tel...
Our R-band data show that the optical light from Malin 1 corresponds well with the >2-arcmin extent ...
none16siThis article has been accepted for publication in MNRAS Letters ©: 2018 The Author(s) Publis...