Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aspc..402..288f&link_type=abstract
Approaching Micro-Arcsecond Resolution with VSOP-2: Astrophysics and Technologies ASP Conference Series, Vol. 402, proceedings o
Astronomy and Astrophysics
Astrophysics
Scientific paper
Radiative transfer in a relativistic vertical wind is examined under the plane-parallel approximation in the fully special relativistic treatment. For an equilibrium flow, where the flow speed and the source function are constant, the relativistic radiative transfer equation is integrated, and the emergent intensity is analytically obtained. In such an equilibrium flow the usual limb-darkening effect does not appear, since the source function is constant. Due to the Doppler and aberration effects associated with the relativistic motion of winds, however, the emergent intensity is strongly enhanced toward the flow direction. This is the relativistic peaking effect. We thus carefully treat and estimate the appearance of relativistic winds and jets, when we observe them in an arbitrary direction.
No associations
LandOfFree
Relativistic Peaking in the Vertical Jets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Relativistic Peaking in the Vertical Jets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relativistic Peaking in the Vertical Jets will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-818291