Search for Galactic Hidden Gas
Farhang Habibi (Orsay
Univ. & SUT)
Abstract:
Primordial cold molecular clouds
may be the ultimate candidates for baryonic hidden
matter in the Galaxy. We have proposed the scintillation
effect of the background stars as a tool to detect
such transparent clouds. An extensive simulation is done
as well as some feasibility tests toward the known dark
nebulae in near infrared band.
I will give a talk about the recent progress of this
investigation.
Wednesday / 7- April-2010 / 18-
Farvardin-1389/ 2:00 PM
IPM Larak Building, School of
Astronomy
Address:
Larak Garden, opposite
Araj, Artesh Highway,Tehran, Iran
E-mail:
astro(at)ipm.ir
