Context. The far-infrared spectra of circumstellar envelopes around various oxygen-rich stars were observed using the ISO Long Wavelength Spectrometer (LWS). These have been shown to be spectrally rich, particularly in water lines, indicating a high H2O abundance. Aims. We have examined high signal-to-noise ISO LWS observations of the luminous supergiant star, VY CM
A low noise (1(sigma) rms approx. 3 mK) 1. nun spectral survey (214.5-285.5 GHz) of the oxygen-rich ...
We present the first far infrared spectra of the Herbig Haro objects HH 52-53-54 and of IRAS 12496-7...
Future IR missions should give some priority to high resolution spectroscopic observations of the se...
Context. The far-infrared spectra of circumstellar envelopes around various oxygen-rich stars were o...
We present 29-197 mu m spectra of the oxygen-rich Mira variable star, R Cas, obtained with the Long-...
We present 29-197 mu m spectra of the oxygen-rich Mira variable star, R Cas, obtained with the Long-...
We present preliminary results of an unbiased spectral survey at 1 mm of the oxygen-rich supergiant,...
The Long Wavelength Spectrometer (LWS) on board the Infrared Space Observatory (ISO) satellite has a...
Aims.The study of the molecular gas in the circumstellar envelopes of evolved stars is normally unde...
Aims. The study of the molecular gas in the circumstellar envelopes of evolved stars is normally und...
Context.Vibrationally excited emission from the SiO and H2O molecules probes the innermost circumst...
The Long-Wavelength Spectrometer (LWS) is one of two complementary spectrometers aboard the European...
Observations of the carbon-bearing molecules CO, HCN, CS, HNC, CN, and HCO+ have been conducted towa...
A complete set of molecular abundances have been established for the Oxygen-rich circumstellar envel...
With the LWS spectrometer on-board the Infrared Space Observatory (ISO), we have detected toward T T...
A low noise (1(sigma) rms approx. 3 mK) 1. nun spectral survey (214.5-285.5 GHz) of the oxygen-rich ...
We present the first far infrared spectra of the Herbig Haro objects HH 52-53-54 and of IRAS 12496-7...
Future IR missions should give some priority to high resolution spectroscopic observations of the se...
Context. The far-infrared spectra of circumstellar envelopes around various oxygen-rich stars were o...
We present 29-197 mu m spectra of the oxygen-rich Mira variable star, R Cas, obtained with the Long-...
We present 29-197 mu m spectra of the oxygen-rich Mira variable star, R Cas, obtained with the Long-...
We present preliminary results of an unbiased spectral survey at 1 mm of the oxygen-rich supergiant,...
The Long Wavelength Spectrometer (LWS) on board the Infrared Space Observatory (ISO) satellite has a...
Aims.The study of the molecular gas in the circumstellar envelopes of evolved stars is normally unde...
Aims. The study of the molecular gas in the circumstellar envelopes of evolved stars is normally und...
Context.Vibrationally excited emission from the SiO and H2O molecules probes the innermost circumst...
The Long-Wavelength Spectrometer (LWS) is one of two complementary spectrometers aboard the European...
Observations of the carbon-bearing molecules CO, HCN, CS, HNC, CN, and HCO+ have been conducted towa...
A complete set of molecular abundances have been established for the Oxygen-rich circumstellar envel...
With the LWS spectrometer on-board the Infrared Space Observatory (ISO), we have detected toward T T...
A low noise (1(sigma) rms approx. 3 mK) 1. nun spectral survey (214.5-285.5 GHz) of the oxygen-rich ...
We present the first far infrared spectra of the Herbig Haro objects HH 52-53-54 and of IRAS 12496-7...
Future IR missions should give some priority to high resolution spectroscopic observations of the se...