We present ISO observations of bright, high-mass southern star-forming regions with the Short Wavelength Spectrometer (SWS) and Long Wavelength Spectrometer (LWS). The selected targets show a range of pre-main sequence evolutionary phases. Whereas some objects still show interstellar ice features, the most evolved objects are coincident with ultracompact HII regions and show strong emission lines from atomic species and polycyclic aromatic hydrocarbons (PAHs). We discuss the ISO spectra between 2.5 - 200 mu m of selected southern star-forming regions in the context of their evolution.</p
The chemical evolution in high-mass star-forming regions is still poorly constrained. Studying the e...
Received xxxx; accepted xxxx The object W33 is a giant molecular cloud that contains star forming re...
Aims.We present SEST observations of the molecular environment ahead of the southern Herbig-Haro obj...
We present ISO observations of bright, high-mass southern star-forming regions with the Short Wavele...
We report on a multi-wavelength (IR to cm) and multi-resolution (1 mas to 20 arcsec) exploration of ...
We report a spectral line survey of the circumstellar envelopes of evolved stars at millimeter wavel...
Abstract. We present 10−15 m spectra of a sample of H ii regions, YSOs and evolved stars that show s...
Massive star formation exhibits an extremely rich chemistry. However, few evolutionary details are k...
Understanding the chemical evolution of young (high-mass) star-forming regions is a central topic in...
A sample of potential massive star-forming regions identified by the 170um ISOPHOT Serendipity Surve...
Abstract. A large fraction of ISO observing time was used to study the late stages of stellar evolut...
We report the results of an investigation, performed with the Long Wavelength Spectrometer (LWS) and...
International audienceAims. Massive stars formin clusters, and they are often found in different evo...
Recent advances in the understanding of the chemical processes that occur during all stages of the f...
Context. Based on color-selected IRAS point sources, we have started to conduct a survey of 47 high-...
The chemical evolution in high-mass star-forming regions is still poorly constrained. Studying the e...
Received xxxx; accepted xxxx The object W33 is a giant molecular cloud that contains star forming re...
Aims.We present SEST observations of the molecular environment ahead of the southern Herbig-Haro obj...
We present ISO observations of bright, high-mass southern star-forming regions with the Short Wavele...
We report on a multi-wavelength (IR to cm) and multi-resolution (1 mas to 20 arcsec) exploration of ...
We report a spectral line survey of the circumstellar envelopes of evolved stars at millimeter wavel...
Abstract. We present 10−15 m spectra of a sample of H ii regions, YSOs and evolved stars that show s...
Massive star formation exhibits an extremely rich chemistry. However, few evolutionary details are k...
Understanding the chemical evolution of young (high-mass) star-forming regions is a central topic in...
A sample of potential massive star-forming regions identified by the 170um ISOPHOT Serendipity Surve...
Abstract. A large fraction of ISO observing time was used to study the late stages of stellar evolut...
We report the results of an investigation, performed with the Long Wavelength Spectrometer (LWS) and...
International audienceAims. Massive stars formin clusters, and they are often found in different evo...
Recent advances in the understanding of the chemical processes that occur during all stages of the f...
Context. Based on color-selected IRAS point sources, we have started to conduct a survey of 47 high-...
The chemical evolution in high-mass star-forming regions is still poorly constrained. Studying the e...
Received xxxx; accepted xxxx The object W33 is a giant molecular cloud that contains star forming re...
Aims.We present SEST observations of the molecular environment ahead of the southern Herbig-Haro obj...