Recent Developments in the Studies of Emission-Line Stars

Details Recent Developments in the Studies of Emission-Line Stars Recent Developments in the Studies of Emission-Line Stars

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008asthe.101..284k&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 101, No. 5, p. 284 - 290 (2008)

Physics

Optics

Emission-Line Stars

Scientific paper

Recent studies of pre-main sequence Ae and Be stars (Herbig Ae/Be stars, or shortly HES) are mainly focused on the imaging of stellar circumstellar disks and the detection and measurements of magnetic fields of these stars. Adaptive optics of Subaru Telescope and infrared interferometric observations in some observatories revealed the complicated structure of stellar disks in different scale of lengths. Magnetic fields of HES suggest the close relationship between magnetic HES and chemically peculiar Ap/Bp stars.

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