In contrast with low-mass young stellar objects (LMYSOs), very little is known about high-mass YSOs (HMYSOs). Latest results indicate that HMYSOs might be born...
TalkThe formation of high mass young stellar objects and the importance of their massive protostellar jets
TalkA GTC survey of exoplanet atmosphere with transmission spectroscopy
Transmission spectroscopy has been a powerful tool to decipher the atmospheric compositions of transiting exoplanets. The recent HST survey has shown that...
PublicationA sixty night campaign on dwarf novae - a progress report.
PublicationA Study of the Photometric and Spectroscopic Variations of the Prototypical FU Orionis-type Star V1057 Cyg
Among the low-mass pre-main sequence stars, a small group called FU Orionis-type objects (FUors) are notable for undergoing powerful accretion outbursts. V1057...
PublicationA suite of community tools for spectro-polarimetric analysis .
The National Center for Atmospheric Research (NCAR) has undertaken a 3-year initiative to develop the Community Spectro-polarimetric Analysis Center (CSAC). The...
NewsA super-Earth is discovered which can be used to test planetary atmosphere models
During the past 25 years astronomers have discovered a wide variety of exoplanets, made of rock, ice and gas, thanks to the construction of astronomical...
TalkA tale of globular clusters formation and evolution. The case of the old, metal-poor globular cluster NGC4372
I will talk about our current understanding of globular cluster (GC) formation and what we have yet to learn about them. I will particularly focus on the...
PublicationAbout the iron carbonyl complex with C60and C70fullerene: [Fe(CO)4(η2C60)] and [Fe(CO)4(η2C70)]
The iron carbonyl complexes with C60 and C70 fullerenes were synthesized in high yield by photochemical irradiation of solutions of C60 and C70 in presence of...
PublicationAbundances of five open clusters (Pancino+, 2010)
Atomic data and equivalent widths for 15 red clump giants in 5 open clusters: Cr 110, NGC 2099, NGC 2420, M 67, NGC 7789. (2 data files).