About: AMBER: Instrument description and first astrophysical results

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Attributs	Valeurs
type	work Issue
Is Part Of	http://hub.abes.fr/edp/periodical/aa/2007/volume_464
Title	AMBER: Instrument description and first astrophysical results
has manifestation of work	http://hub.abes.fr/edp/periodical/aa/2007/volume_464/issue_1/m/print http://hub.abes.fr/edp/periodical/aa/2007/volume_464/issue_1/m/web
publisher identifier	aa/2007/10
issue	1
is Is Part Of of	The VLT-FLAMES survey of massive stars: observations centered on the Magellanic Cloud clusters NGC 330, NGC 346, NGC 2004, and the N11 region Direct constraint on the distance of γ2 Velorum from AMBER/VLTI observations Primary particle acceleration above 100 TeV in the shell-type supernova remnant RX J1713.7-3946 with deep HESS observations X-ray broad-band study of the symbiotic X-ray binary 4U 1954+31 AMBER/VLTI interferometric observations of the recurrent Nova RS Ophiuchii 5.5 days after outburst Deep imaging survey of the environment of α Centauri EDITORIAL Beam mismatch effects in cosmic microwave background polarization measurements Spectral types of planetary host star candidates from OGLE III Optical configuration and analysis of the AMBER/VLTI instrument AMBER, the near-infrared spectro-interferometric three-telescope VLTI instrument Deuterium fractionation in warm dense interstellar clumps HD 143418: an unusual light variable and a double-lined spectroscopic binary with a CP primary Disk and wind interaction in the young stellar object MWC 297 spatially resolved with AMBER/VLTI Interferometric data reduction with AMBER/VLTI. Principle, estimators, and illustration An asymmetry detected in the disk of κ Canis Majoris with AMBER/VLTI Proper-motion binaries in the Hipparcos catalogue Chandra observation of the dipping source XB 1254-690 Barred CO emission in HE 1029-1831 How does the shape and thickness of the tachocline affect the distribution of the toroidal magnetic fields in the solar dynamo? Unveiling the Cygnus OB2 stellar population with Chandra Why your model parameter confidences might be too optimistic. Unbiased estimation of the inverse covariance matrix Photodissociation of organic molecules in star-forming regions Multi-frequency monitoring of γ-ray loud blazars Carbamic acid produced by the UV/EUV irradiation of interstellar ice analogs Stars and gas in the very large interacting galaxy NGC 6872 High-resolution spectroscopy of RGB stars in the Sagittarius streams GeV-TeV $\vec{\gamma}$-ray light curves expected in the IC e $^\pm$ pair cascade model for massive binaries: application to LS 5039 Buoyant bubbles in a cooling intracluster medium The diocotron instability in a pulsar cylindrical electrosphere Modeling the UBVRI time delays in Mrk 335 AMBER/VLTI and MIDI/VLTI spectro-interferometric observations of the B[e] supergiant CPD $-57\mathrm{^\circ}\,2874$ UNNOFIT inversion of spectro-polarimetric maps observed with THEMIS First direct detection of a Keplerian rotating disk around the Be star $\mathsf{\alpha}$ Arae using AMBER/VLTI Near-infrared interferometry of η Carinae with spectral resolutions of 1 500 and 12 000 using AMBER/VLTI Determination of field strengths in the quiet Sun Constraining the wind launching region in Herbig Ae stars: AMBER/VLTI spectroscopy of HD 104237 Compositional dependence of infrared absorption spectra of crystalline silicates The hot subdwarf B + white dwarf binary KPD 1930+2752 Poynting-Robertson effect and perihelion motion Six large coronal X-ray flares observed with Chandra Overluminous HNC line emission in Arp 220, NGC 4418 and Mrk 231. Global IR pumping or XDRs? An empirical 3D model of the large-scale coronal structure based on the distribution of H α filaments on the solar disk

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