We have undertaken a comprehensive search for the first excited state of OH emission (J=5/2, 2?3/2) in Planetary and Proto- Planetary Nebulae. With the Effelsberg telescope, we confirm the detection of Vy 2?2 and we present one new detection in the pPN K3?35. This detection has been confirmed by subsequent observations made at 6035 MHz with the MERLIN interferometer. This is the first detection of 6 GHz OH maser emission from a post-AGB star
Context. Maser emission is a strong tool for studying high-mass star-forming regions and their evolu...
International audienceWe present a study of 18 cm OH maser emission toward 20 high-mass young stella...
Aims. We report the first detections of OH+ emission in planetary nebulae (PNe). Methods. As part of...
International audienceWe have undertaken a comprehensive search for the first excited state of OH em...
International audienceAims: The aim of this study is to investigate the physical properties of molec...
Aims. The aim of this study is to investigate the physical properties of molecular envelopes of plan...
Aims. The aim of this study is to investigate the physical properties of molecular envelopes of plan...
We report on OH maser emission toward G336.644-0.695 (IRAS 16333-4807), which is a H2O maser-emittin...
We report on OH maser emission toward G336.644-0.695 (IRAS 16333-4807), which is a H₂O maser-emittin...
We present a survey for OH maser emission at 18 cm in the direction of 196 IRAS point sources. The ...
We have undertaken a comprehensive search for 5-cm excited OH maser emission from evolved stars repr...
Aims. We studied the characteristics of planetary nebulae (PNe) that show both OH maser and radio co...
This thesis reports the calibration, imaging and analysis of one epoch of VLBA observations of the 1...
Measurements of the sizes and spatial distribution of the source of OH emission at 1665 MHz near the...
© 2016. The American Astronomical Society. All rights reserved. We report on OH maser emission towar...
Context. Maser emission is a strong tool for studying high-mass star-forming regions and their evolu...
International audienceWe present a study of 18 cm OH maser emission toward 20 high-mass young stella...
Aims. We report the first detections of OH+ emission in planetary nebulae (PNe). Methods. As part of...
International audienceWe have undertaken a comprehensive search for the first excited state of OH em...
International audienceAims: The aim of this study is to investigate the physical properties of molec...
Aims. The aim of this study is to investigate the physical properties of molecular envelopes of plan...
Aims. The aim of this study is to investigate the physical properties of molecular envelopes of plan...
We report on OH maser emission toward G336.644-0.695 (IRAS 16333-4807), which is a H2O maser-emittin...
We report on OH maser emission toward G336.644-0.695 (IRAS 16333-4807), which is a H₂O maser-emittin...
We present a survey for OH maser emission at 18 cm in the direction of 196 IRAS point sources. The ...
We have undertaken a comprehensive search for 5-cm excited OH maser emission from evolved stars repr...
Aims. We studied the characteristics of planetary nebulae (PNe) that show both OH maser and radio co...
This thesis reports the calibration, imaging and analysis of one epoch of VLBA observations of the 1...
Measurements of the sizes and spatial distribution of the source of OH emission at 1665 MHz near the...
© 2016. The American Astronomical Society. All rights reserved. We report on OH maser emission towar...
Context. Maser emission is a strong tool for studying high-mass star-forming regions and their evolu...
International audienceWe present a study of 18 cm OH maser emission toward 20 high-mass young stella...
Aims. We report the first detections of OH+ emission in planetary nebulae (PNe). Methods. As part of...