Home ContactSitemap CAS中文
About Us
Brief Introduction
History
Directors
Organization
Research Groups
Scientific Progress
Seminars
Colloquia
CAS Members
Experts
Faculty
Research Fields
Center for Astro-geodynamics
Astrophysics Division
DRAST (Division of Radio Astronomy Science and Technology )
High Technology Laboratories

Location: Home>Research>Seminars
Multi-wavelength Time Domain Astronomy: To Probe the Environs of Central Super Massive Black Hole of Blazars
Author:
ArticleSource:
Update time: 2017-03-17
Close
Text Size: A A A
Print

Title: Multi-wavelength Time Domain Astronomy: To Probe the Environs of Central Super Massive Black Hole of Blazars  

Speaker: Alok C. Gupta (ARIES/SHAO)   

Time: 3 PM, Mar. 23th (Thursday)     

Location: Lecture Hall, 3rd floor     

Abstract:   

This is the age of multi-wavelenth time domain astronomy in which the transient astronomical sources are of great interest due to their rapid change in flux and polarization. Simultaneous multi-wavelength observation of a particular transient source on an extended period of time has importance to understand the emission mechanism in different electromagnetic bands. Blazars are among one of the most favorite astronomical transient objects, because they emit radiation in the complete electromagnetic spectrum, and their flux and polarization are highly variable.  

In the present talk, I will summarize our recent results based on multi-wavelength observations taken with space and ground based telescopes.  The scientific projects involve are: multi-wavelength flux, polarization and cross-correlated variability of blazars on diverse timescales, and optical and X-ray QPOs in blazars.   

Shanghai Astronomical Observatory, All Rights Reserved
80 Nandan Road, Shanghai 200030, China
Tel: +86-21-64386191 Email:shao@shao.ac.cn