Astronomy and Astrophysics Seminars

Studies of massive star forming regions at infrared wavelengths

by Dr. Watson P. Varricatt (United Kingdom Infrared Telescope, Hawaii, USA.)

Tuesday, July 7, 2015 from to (Asia/Kolkata)
at TIFR ( DAA Seminar A269 )
Description
Low-mass stars are known to form primarily through disk accretion.
When it comes to massive stars, this has been a debated topic. The
objections to accretion as the leading mechanism came from
observational and theoretical considerations, and alternative
scenarios like merger of lower mass stars were proposed. However,
recent observational studies show evidence for objects up to at least
late-O spectral types forming through disk accretion. We  have been
observing massive star forming regions using the United Kingdom
Infrared Telescope to understand the mechanisms leading to their
formation. In this talk, I will present some of the interesting results
from our studies.