Contact | Site Map | CAS

中文 Home About Us Research News People Education Publications Resources International Cooperation Join Us
News
Header Lines
NAOC News
Research Progress
International Cooperation News
Seminars & Colloquia
Upcoming Events
Conferences & Workshops
  Location:Home>News>Seminars & Colloquia
Herschel's view of low-mass star formation (NAOC colloquium_No.09/2012) TEXT SIZE: A A A

国台学术报告 NAOC COLLOQUIUM

2012年 第09次 / Number 09, 2012

Speaker: Dr. Greg Herczeg (KIAA)
Time: Wednesday, 3:00 PM, Mar. 14, 2012 
Location: NAOC A601

 

Dr. Greg Herczeg is a Bairen Research Professor at Kavli Institute for Astronomy and Astrophysics, Peking University. He did his Ph.D at the University of Colorado. He was a postdoctoroal scholar at Caltech since 2005. His research interest lies primarily in Accretion onto young stars, disk dissipation mechanisms and disk structure, observational diagnostics of wind launching mechanisms, pre-main sequence stellar evolution, chromospheric and coronal activity around dwarf stars.

 

 

 

 

 

Abstract: The Herschel Space Observatory is currently providing an unprecedented view of the far-infrared sky.  Herschel's unique spectral and imaging capabilities in this key wavelength region are revolutionizing our views of star and planet formation.  In this talk, I will review how Herschel has changed our understanding of pre-main sequence stellar evolution, including the structure of cold molecular clouds and initial collapse of a protostar, feedback between the star and surrounding envelope, and the structure and chemistry of proto-planetary disks. 

 

 

 

All are welcome!Tea, coffee, biscuits will be served at 2:45 P.M.

Copyright @2005-2015,     National Astronomical Observatories, Chinese Academy of Sciences
20A Datun Road, Chaoyang District, Beijing, China
Tel:010-64888708    E-mail: ccz@bao.ac.cn