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SF2A-2013: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics

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The article was published on 2013-11-01 and is currently open access. It has received 230 citations till now.

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Journal ArticleDOI

Variation of the FIR/submm optical properties of silicate dust analogues at low temperature: Implications for the observations of interstellar cold dust emission

TL;DR: In this paper, the authors present results from experimental studies aiming at measuring the Mass Absorption Coefficient (MAC) of interstellar silicate dust analogues at low temperatures in the far infrared and submillimetre domains which are necessary for the analysis of astronomical data.
Journal ArticleDOI

Planet forming disks, debris disks and the Solar System

Inga Kamp
TL;DR: In this paper, the synergy between disk structure/evolution modeling and astrochemical laboratory/theoretical work is discussed, highlighting the most recent advances and open questions such as how much of the chemical composition in disks is inherited from molecular clouds, the relevance of snowlines for planet formation, and what is the origin of the gas in debris disks and what can we learn from it.
Book ChapterDOI

Introduction: The Hunt for Extra-Solar Planets

TL;DR: In the last few decades, developments in instrumentation and observation techniques have led to revolutionary discoveries: we now know that planets revolving around other stars than our Sun exist, and better still, they appear to be very common.

METEOSPACE, solar monitoring and space weather at Calern observatory

TL;DR: METEOSPACE as discussed by the authors is a new partnership project between the Paris Observatory, the Observatoire de la Cote d'Azur (OCA), the French Air Force and a service company (LUNA technology) for the development and operation of a set of small telescopes Hα / Ca II K/ Ca II H / G band to be installed at on the Calern plateau.
Journal ArticleDOI

Search for gravitational redshifted absorption lines in LMXB Serpens X-1.

TL;DR: In this article, the authors search for redshifted lines in the persistent emission, where the accretion flow dominates over the surface emission, and show that narrow absorption lines from highly ionized iron can potentially be observable in accreting low-mass X-ray binaries (LMXBs; low B field) that have either low spin or low inclination so that Doppler broadening is small.
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