Near Infrared High Angular Resolution Imaging of Young Stellar Objects

Details Near Infrared High Angular Resolution Imaging of Young Stellar Objects Near Infrared High Angular Resolution Imaging of Young Stellar Objects

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cokon.100..363a&link_type=abstract

Communications of the Konkoly Observatory, No. 100 (Vol. XII, 2), p. 363-368 (1997)

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The use of high angular resolution (HAR) techniques to observe young stellar objects (YSOs) corresponds to the wish to resolve disk-like structures around these objects. Such structures are well expected features of young stars. The near infrared is well suited to the study of the circumstellar environment (at these wavelengths, the optical depth is much smaller than in optical). Here I present near infrared HAR imaging methods. I will point out the advantage of each observing mode and will comment, on the basis of few examples, the results of such observations. Among others, the impact of the discovered high degree of multiplicity of YSOs will be discussed.

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