Add to ORKGThe analysis and interpretation of molecular line data from the interstellar medium, and more specifically from regions of star formation, is bound to grow in importance over the coming decade with the upcoming Herschel Space Observatory and ALMA interferometer. In this dissertation, a newly developed three-dimensional code is presented that solves radiative transfer problems pertinent to the excitation of water lines. The code is used to study the emissivity of water in star-forming regions
The spatial origin and detectability of rotational H(2)O emission lines from Herbig Ae type protopla...
Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it i...
Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it i...
The analysis and interpretation of molecular line data from the interstellar medium, and more specif...
H(2)O is a key ingredient in many interstellar environments, like photon dominated regions and star ...
$\mathrm{H_2O}$ is a key ingredient in many interstellar environments, like photon dominated regions...
Context. Within low-mass star formation, water vapor plays a key role in the chemistry and energy b...
Context. Observations of water lines are a sensitive probe of the geometry, dynamics and chemical st...
Context.Observations of water lines are a sensitive probe of the geometry, dynamics and chemical str...
Context. Apart from being an important coolant, water is known to be a tracer of high-velocity molec...
In this research water emission is modeled from intermediate mass star formations regions placed at ...
Context. Water is a key tracer of dynamics and chemistry in low-mass star-forming regions, but spect...
This paper reviews recent observations of water in Galactic interstellar clouds and nearby galactic ...
The spatial origin and detectability of rotational H(2)O emission lines from Herbig Ae type protopla...
Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it i...
Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it i...
The analysis and interpretation of molecular line data from the interstellar medium, and more specif...
H(2)O is a key ingredient in many interstellar environments, like photon dominated regions and star ...
$\mathrm{H_2O}$ is a key ingredient in many interstellar environments, like photon dominated regions...
Context. Within low-mass star formation, water vapor plays a key role in the chemistry and energy b...
Context. Observations of water lines are a sensitive probe of the geometry, dynamics and chemical st...
Context.Observations of water lines are a sensitive probe of the geometry, dynamics and chemical str...
Context. Apart from being an important coolant, water is known to be a tracer of high-velocity molec...
In this research water emission is modeled from intermediate mass star formations regions placed at ...
Context. Water is a key tracer of dynamics and chemistry in low-mass star-forming regions, but spect...
This paper reviews recent observations of water in Galactic interstellar clouds and nearby galactic ...
The spatial origin and detectability of rotational H(2)O emission lines from Herbig Ae type protopla...
Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it i...
Context. Water is a key molecule in the physics and chemistry of star and planet formation, but it i...