Topics
H IISettlement
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Hubble Space Telescope (HST)Societal event
HSTSocietal event
H II regionSettlement
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The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass distribution of OB associations and is an excellent tracer of the newly formed massive stars and associations. To date, extensive work (predominantly in Hα) has been done from the ground, which is hindered by dust extinction and the severe blending of adjacent (spatially or in projection) H II regions. Reliably measuring the properties of H II regions requires a linear resolution <40 pc, but analyses satisfying this requirement have been done only in a handful of galaxies, so far. As the first space-based work using a galaxy sample, we have selected 12 galaxies from our HST/NICMOS Paα survey and studied the LF and size distribution of H II reg...
A study is presented of the H II region luminosity function (LF) of M51, complete down to a luminosi...
We analyze the statistical properties of the circumnuclear H II regions of a sample of 52 nearby gal...
To derive a new H alpha luminosity function and to understand the clustering properties of star-form...
The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass d...
Two continuum subtracted H-alpha HST frames of M101 are used to determine the positions, angular siz...
We have re-analyzed continuum and recombination lines radio data available in the literature in orde...
International audienceWe use an unprecedented sample of about 23 000 H II regions detected at an ave...
Observed variations in the HII region luminosity function (HII LF) seen in spiral arm vs. interarm r...
(Abridged) From a new H alpha mosaic image of the complete disc of the spiral galaxy M100, a catalog...
We use an unprecedented sample of about 23 000 H II regions detected at an average physical resoluti...
We examine from a theoretical viewpoint how the physical parameters of H II regions are controlled b...
Using B , R and HΑ images of roughly equal-sized samples of low surface brightness (LSB) and high su...
An infrared survey of the central 650 arcmin$^2$ of the Coma cluster is used to determine the $H$ ba...
We use an unprecedented sample of about 23 000 H II regions detected at an average physical resoluti...
We present HST/WFC3 narrowband imaging of the Hα emission in a sample of eight gravitationally-lense...
A study is presented of the H II region luminosity function (LF) of M51, complete down to a luminosi...
We analyze the statistical properties of the circumnuclear H II regions of a sample of 52 nearby gal...
To derive a new H alpha luminosity function and to understand the clustering properties of star-form...
The H II region luminosity function (LF) is an important tool for deriving the birthrates and mass d...
Two continuum subtracted H-alpha HST frames of M101 are used to determine the positions, angular siz...
We have re-analyzed continuum and recombination lines radio data available in the literature in orde...
International audienceWe use an unprecedented sample of about 23 000 H II regions detected at an ave...
Observed variations in the HII region luminosity function (HII LF) seen in spiral arm vs. interarm r...
(Abridged) From a new H alpha mosaic image of the complete disc of the spiral galaxy M100, a catalog...
We use an unprecedented sample of about 23 000 H II regions detected at an average physical resoluti...
We examine from a theoretical viewpoint how the physical parameters of H II regions are controlled b...
Using B , R and HΑ images of roughly equal-sized samples of low surface brightness (LSB) and high su...
An infrared survey of the central 650 arcmin$^2$ of the Coma cluster is used to determine the $H$ ba...
We use an unprecedented sample of about 23 000 H II regions detected at an average physical resoluti...
We present HST/WFC3 narrowband imaging of the Hα emission in a sample of eight gravitationally-lense...
A study is presented of the H II region luminosity function (LF) of M51, complete down to a luminosi...
We analyze the statistical properties of the circumnuclear H II regions of a sample of 52 nearby gal...
To derive a new H alpha luminosity function and to understand the clustering properties of star-form...
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