Convectively driven vortex flows in the Sun
Not Available
Bonet, J. A. et al.
Advertised on:
10
2008
This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..
It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/
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Cool atmosphere models and observations: liability and limits of brown dwarfs and exoplanets physical parameters determination
The study of cool atmospheres is currently a fruitful field of interaction between theorists developing better atmosphere models and observers discovering new cool objects and analysing their emission spectrum. Save for a few close binaries with known parallax and a dynamical mass determination, comparison of spectra to models is the only method
Delorme, P. et al.Advertised on:
102010 -
Cooling of the quasi-persistent neutron star X-ray transients KS 1731-260 and MXB 1659-29
We present Chandra and XMM-Newton X-ray observations that monitor the neutron star cooling of the quasi-persistent neutron star X-ray transients KS 1731-260 and MXB 1659-29 for approximately 4 yr after these sources returned to quiescence from prolonged outbursts. In both sources the outbursts were long enough to significantly heat the neutron star
Cackett, Edward M. et al.Advertised on:
102006 -
CoRoT Highlights in exoplanetology
The CoRoT satellite is the first instrument hunting for planets from space. We will review the status of the CoRoT/Exoplanet program. We will then present the CoRoT exoplanetary systems and how they widen the range of exoplanet properties and contribute to our understanding of these objects.
Moutou, C. et al.Advertised on:
102011 -
CoRoT LRa02_E2_0121: Neptune-size planet candidate turns into a hierarchical triple system with a giant primary
This paper presents the case of CoRoT LRa02_E2_0121, which was initially classified as a Neptune-size transiting-planet candidate on a relatively wide orbit of 36.3 days. Follow-up observations were performed with UVES, Sandiford, SOPHIE, and HARPS. These observations revealed a faint companion in the spectra. To find the true nature of the system
Tal-Or, L. et al.Advertised on:
102011 -
CoRoT Measures Solar-Like Oscillations and Granulation in Stars Hotter Than the Sun
Oscillations of the Sun have been used to understand its interior structure. The extension of similar studies to more distant stars has raised many difficulties despite the strong efforts of the international community over the past decades. The CoRoT (Convection Rotation and Planetary Transits) satellite, launched in December 2006, has now
Michel, Eric et al.Advertised on:
102008