The spatial origin and detectability of rotational H2O emission lines from Herbig Ae type protoplanetary disks beyond 70 μm is discussed. We use the recently developed disk code prodimo
Observationally locating the position of the H2O snowline (e.g., Hayashi et al. 1981, 1985) in proto...
Observationally locating the position of the H2O snowline (=the sublimation front of water molecules...
Water plays a fundamental role in the formation of planets and their atmospheres. Far-infrared obser...
The spatial origin and detectability of rotational H(2)O emission lines from Herbig Ae type protopla...
Protoplanetary disks represent the stage between the pre-stellar collapse of the molecolar cloud and...
Circumstellar disks provide the material reservoir for the growth of young stars and for planet form...
We present observations of far-infrared (50-200 mu m) OH and H2O emission of the disk around the Her...
Context. This paper discusses the sensitivity of water lines to chemical processes and radiative tra...
We present high-resolution (R similar to 100,000) L-band spectroscopy of 11 Herbig AeBe stars with c...
Context. This paper discusses the sensitivity of water lines to chemical processes and radiative tra...
Observationally locating the position of the H2O snowline (e.g., Hayashi et al. 1981, 1985) in proto...
Observationally locating the position of the H2O snowline (=the sublimation front of water molecules...
Water plays a fundamental role in the formation of planets and their atmospheres. Far-infrared obser...
The spatial origin and detectability of rotational H(2)O emission lines from Herbig Ae type protopla...
Protoplanetary disks represent the stage between the pre-stellar collapse of the molecolar cloud and...
Circumstellar disks provide the material reservoir for the growth of young stars and for planet form...
We present observations of far-infrared (50-200 mu m) OH and H2O emission of the disk around the Her...
Context. This paper discusses the sensitivity of water lines to chemical processes and radiative tra...
We present high-resolution (R similar to 100,000) L-band spectroscopy of 11 Herbig AeBe stars with c...
Context. This paper discusses the sensitivity of water lines to chemical processes and radiative tra...
Observationally locating the position of the H2O snowline (e.g., Hayashi et al. 1981, 1985) in proto...
Observationally locating the position of the H2O snowline (=the sublimation front of water molecules...
Water plays a fundamental role in the formation of planets and their atmospheres. Far-infrared obser...
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