Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012aas...21934308t&link_type=abstract
American Astronomical Society, AAS Meeting #219, #343.08
Astronomy and Astrophysics
Astronomy
Scientific paper
We present Far-UV continuum map of the Taurus-Auriga-Perseus(TPA) complex, one of the largest local associations of dark cloud located in (l, b)=([152,180], [-28, 0]), using both FIMS/SPEAR and GALEX. We also present the result of FUV dust scattering simulation in the same region, which is based on Monte Carlo Radiative Transfer(MCRT) technique. We basically assume that scattered starlight is the most prominent component of FUV continuum in this region. From the assumption we compare our scattering simulation results to FIMS-GALEX unified FUV continuum and then through that we prove the spatial distribution of the complex region. The simulation results reveal as well their own scattering properties such as albedo(a) and asymmetry factor(g) in the whole TAP region at 1565A. We compare the results above to some previous studies related to this region including effective distance of dark clouds, dust density and dust distribution.
Min Kyoung
Seon Kwangil
Tae-Ho Lim
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