NIR high-resolution imaging of young stars

Details NIR high-resolution imaging of young stars NIR high-resolution imaging of young stars

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994inpht..35..487s&link_type=abstract

Infrared Physics & Technology, Volume 35, Issue 2-3, p. 487-491.

Physics

6

Scientific paper

High resolution imaging of young stellar objects (YSOs) in the near-infrared wavelength region (NIR) can reveal the spatial distribution of warm circumstellar dust as well as the multiplicity of the sources. We investigated a sample of southern Herbig Ae/Be stars, Vega-type stars, and a region in the Hourglass nebula with high spatial resolution. For most of the objects, the observations yielded diffraction limited resolution (0.15'' in the K band). In this contribution, we report on first results for the Herbig Ae/Be star HR 5999, the Chamaeleon Infrared Nebula (IRN), and the exciting star of the Hourglass nebula, Herschel 36.

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