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  1. No Access

    Article

    Two families of exocomets in the β Pictoris system

    Statistical analysis of over a thousand spectra of the star β Pictoris reveals that it has two kinds of exocomets circling it: old exhausted comets trapped in mean-motion resonance with a massive planet, and f...

    F. Kiefer, A. Lecavelier des Etangs, J. Boissier, A. Vidal-Madjar, H. Beust in Nature (2014)

  2. Article

    The origin of hydrogen around HD 209458b

    Arising from: M. Holmström et al. Nature 451, 970–972 (2008)10.1038/nature06600; Holmström et al. reply

    A. Lecavelier des Etangs, A. Vidal-Madjar, J.-M. Désert in Nature (2008)

  3. No Access

    Article

    An extended upper atmosphere around the extrasolar planet HD209458b

    The planet in the system HD209458 is the first one for which repeated transits across the stellar disk have been observed1,2. Together with radial velocity measurements3, this has led to a determination of the pl...

    A. Vidal-Madjar, A. Lecavelier des Etangs, J.-M. Désert, G. E. Ballester in Nature (2003)

  4. No Access

    Chapter

    Lyman Gamma Satellites Due to H-H+ Collisions: Application to FUSE Observations of Hot White Dwarfs

    New theoretical calculations of Lyman 7 profiles perturbed by protons allow us to identificate a large feature near 995 Å in FUSE observations of hot white dwarfs. This feature is due to quasi-molecular Lyman ...

    N. F. Allard, S. Bourdreux, J. F. Kielkopf, G. Hébrard, J.-M. Désert in White Dwarfs (2003)

  5. No Access

    Chapter

    Quasi-Molecular Lines in Lyman Wings of Cool DA White Dwarfs; Application to FUSE Observations of G 231–40

    We present new theoretical calculations of Lyman β profiles which include perturbations by both neutral hydrogen and protons. They are used to improve theoretical modeling of synthetic spectra for cool DA white d...

    N. F. Allard, G. Hébrard, R. Ferlet, A. Vidal-Madjar, I. Hubeny, S. Lacour in White Dwarfs (2003)

  6. No Access

    Article

    Deficiency of molecular hydrogen in the disk of β Pictoris

    Molecular hydrogen (H2) is by far the most abundant material from which stars, protoplanetary disks and giant planets form, but it is difficult to detect directly. Infrared emission lines from H2 have recently be...

    A. Lecavelier des Etangs, A. Vidal-Madjar, A. Roberge, P. D. Feldman, M. Deleuil in Nature (2001)

  7. No Access

    Article

    New Observations of Galactic Deuterium

    G. Sonneborn, E.B. Jenkins, T. Tripp, P. Wozniak in Astrophysics and Space Science (1999)

  8. No Access

    Chapter and Conference Paper

    New Observations of Galactic Deuterium

    Observations made with the Interstellar Medium Absorption Profile Spectrograph (IMAPS) on the US-German ORFEUS-SPAS II mission in late 1996 provide the first new measurements of Galactic interstellar atomic de...

    G. Sonneborn, E. B. Jenkins, T. Tripp in Galaxy Evolution: Connecting the Distant U… (1999)

  9. No Access

    Article

    Deuterium Observations in the Galaxy

    An accurate measurement of the primordial value of D/H would provide one of the best tests of nucleosynthesis models for the early Universe and the baryon density. Such evaluations have been traditionally made...

    A. Vidal-Madjar, R. Ferlet, M. Lemoine in Space Science Reviews (1998)

  10. No Access

    Chapter and Conference Paper

    The Two EROS 4k x 8k CCD Mosaic Cameras

    We present our new astronomical wide field imager, which consists of two 4k x 8k CCD mosaic cameras allowing simultaneous imaging in two focal planes with different color passbands. Each mosaic is maintained a...

    F. Bauer, J. De Kat, C. Afonso, E. Aubourg, S. Aune in Optical Detectors for Astronomy (1998)

  11. No Access

    Chapter and Conference Paper

    Deuterium Observations in the Galaxy

    An accurate measurement of the primordial value of D/H would provide one of the best tests of nucleosynthesis models for the early Universe and the baryon density. Such evaluations have been traditionally made...

    A. Vidal-Madjar, R. Ferlet, M. Lemoine in Primordial Nuclei and Their Galactic Evolution (1998)

  12. No Access

    Article

    A high deuterium abundance at redshift z = 0.7

    Of the light elements, the primordial abundance of deuterium relative to hydrogen, (D/H)p, provides the most sensitive diagnostic1 for the cosmological mass density parameter, ΩB. Recent high-redshift D/H measure...

    J. K. Webb, R. F. Carswell, K. M. Lanzetta, R. Ferlet, M. Lemoine in Nature (1997)

  13. No Access

    Chapter and Conference Paper

    The Interstellar Gas in the Line of Sight to ε Canis Majoris

    We analyse Hubble Space Telescope GHRS observations of the interstellar medium in the direction to ε CMa, the strongest EUV source in the sky located 200 pc away in a region deficient in neutral gas. We show that...

    C. Gry, L. Lemonon, A. Vidal-Madjar, M. Lemoine in Astrophysics in the Extreme Ultraviolet (1996)

  14. No Access

    Article

    A 20 cm2 CCD mosaic camera for a dark matter search part I : Mechanics, optics and cryogeny

    A 20cm 2 CCD mosaic camera has been especially built to search for dark galactic halo objects by the gravitational microlensing effect. The sensitive area is made of 16 edge-bu...

    M. Arnaud, E. Aubourg, P. Bareyre, S. Br';ehin, R. Caridroit in Experimental Astronomy (1994)

  15. No Access

    Article

    A 20cm 2 CCD mosaic camera for a dark matter search part II : Electronics, data acquisition and performance

    To summarize, the readout and the control system of the CCD mosaic camera are running since December 1991 at the La Silla Observatory (ESO). The overall performance of the camera has been good. About 12000 pic...

    M. Arnaud, E. Aubourg, P. Bareyre, S. Br';ehin, R. Caridroit in Experimental Astronomy (1994)

  16. No Access

    Article

    Cometary-like bodies in the protoplanetary disk aroundβ pictoris

    Repeated spectroscopic observations ofβ Pictoris have been performed since 1985 and revealed the presence, in many metallic lines likeCa II, Mg II, Fe II, ..., of strong sporadic circumstellar absorption, redshif...

    H. Beust, A. Vidal-Madjar, R. Ferlet in Astrophysics and Space Science (1994)

  17. No Access

    Article

    Inner part observation of theβ pictoris disk

    The inner regions of the circumstellar disk aroundβ Pictoris might be dust-free due to a possible planet which may have cleared up dust particles. We present a new observational technique based on the use of an a...

    R. Ferlet, A. Lecavelier Des Etangs, G. Perrin in Astrophysics and Space Science (1994)

  18. No Access

    Chapter and Conference Paper

    Cometary-Like Bodies in the Protoplanetary Disk Around β Pictoris

    Repeated spectroscopic observations of β Pictoris have been performed since 1985 and revealed the presence, in many metallic lines like Ca II, Mg II, Fe II, …, of strong sporadic circumstellar absorption, reds...

    H. Beust, A. Vidal-Madjar, R. Ferlet in Planetary Systems: Formation, Evolution, a… (1994)

  19. No Access

    Chapter and Conference Paper

    Inner Part Observation of the β Pictoris Disk

    The inner regions of the circumstellar disk around β Pictoris might be dust-free due to a possible planet which may have cleared up dust particles. We present a new observational technique based on the use of ...

    R. Ferlet, A. Lecavelier Des Etangs in Planetary Systems: Formation, Evolution, a… (1994)

  20. No Access

    Article

    Evidence for gravitational microlensing by dark objects in the Galactic halo

    THE flat rotation curves of spiral galaxies, including our own, indicate that

    E. Aubourg, P. Bareyre, S. Bréhin, M. Gros, M. Lachièze-Rey, B. Laurent in Nature (1993)

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