Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...211.5710q&link_type=abstract
American Astronomical Society, AAS Meeting #211, #57.10; Bulletin of the American Astronomical Society, Vol. 39, p.831
Astronomy and Astrophysics
Astrophysics
Scientific paper
We present observations of MWC\,349\,A with MIDI at the VLTI (the Mid-Infrared Interferometric Instrument at ESO's Very Large Telescope Interferometer), which are a prime example of the power of combined spatial and spectral resolution for addressing complex astrophysical phenomena.
Previous observations of the peculiar emission line star MWC\,349\,A suggest that it is a young massive star in the short-lived phase when the parental cloud has been completely dispersed, but the accretion disk has not yet been destroyed by ionization. The system is seen nearly edge-on; the unique hydrogen recombination line maser / laser activity of MWC\,349\,A from mm to infrared wavelengths is likely a consequence of this viewing geometry.
We have taken 13 measurements with MIDI at the VLTI (Very Large Telescope Interferometer) in the GRISM mode covering the N band (8 to 13 microns) at a spectral resolution R ≈ 230. The wavelength dependence of the continuum visibility agrees with model calculations for circumstellar dust disks. In addition, the signatures of at least a dozen emission lines have been identified in the interferometric data.
We present a first analysis of visibility amplitudes and differential phase data. In particular we show that a simple model can represent the SED and visibility amplitudes of the continuum flux. The visibilities for the hydrogen and forbidden lines are also discussed.
Albrecht Simon
Quirrenbach Andreas
Tubbs Robert N.
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