Near-infrared photometric monitoring of a pre-main-sequence object KH 15D

Details Near-infrared photometric monitoring of a pre-main-sequence object KH 15D Near-infrared photometric monitoring of a pre-main-sequence object KH 15D

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006asthe..99..365k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 99, No. 7, p. 365 - 371 (2006)

Astronomy and Astrophysics

Astronomy

Pre-Main-Sequence Stars, Infrared Photometry

Scientific paper

An extensive photometric monitoring of KH 15D has been conducted. The infrared variability is characterized by large-amplitude and long-lasting eclipse, as observed at optical. The blueing of the J-H color during the eclipse, which has been suggested before, is unambiguously confirmed. Most of these variability features of KH 15D observed at near-infrared wavelengths can be explained with the recent model employing an eclipse by the inclined, processing disk and an outer scattering region around a pre-main-sequence binary.

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