Multiplicity of Herbig Ae/Be Stars
Project Home Page
Herbig Ae/Be stars
Herbig Ae/Be stars are pre-main sequence stars of intermediate mass,
with masses between 2 and 8 Msun.
Their characteristics are:
- spectral type B through F
- IR excess
- emission lines
and as such they are the link between low-mass PMS stars and high-mass
PMS stars.
Publications and presentations
Posters presented at the January 2007 AAS:
- AO Imageing Survey:
- Spectroscopic results:
IAU Symposiom 240, August 2006:
- Multiplicity of Herbig Ae/Be stars -- PDF
Posters presented at the January 2006 AAS:
- An overview of the project:
- First results:
Protostars and Planets V, October 2005:
- Spectroscopic Follow-Up of HAEBE Binaries-- PDF
Students
Several CTIO REU/PIA students have contributed to this project,
and results of their work can be found in the
HAEBE Student Pages.
This summer Claudia Araya from the Pontificia Universidad Catolica de
Chile will be working with us.
Team
To go to the members only pages, click
here .
January 15, 2007