New constraints on the dust surrounding HR 4796A | Astronomy & Astrophysics (A&A)

Free Access

Table 7

Posterior probability of H₁ (the NW is inclined towards the Earth) and H₂ given different observables, using the Mie theory.


Observable	Ψ(H₁ \| observable)	Ψ(H₂ \| observable)

p	28.1%	71.9%
p × φ	>99.9%	<0.1%
φ	16.9%	83.1%
scat. light^a	>99.9%	<0.1%
overall^b	>99.9%	<0.1%

Notes. The shaded row highlights the overall conclusion.

^(a)

Includes the following independent scattered light observables: polarised fraction p, polarised phase function p × φ, effective albedo and colour index.

^(b)

Includes the SED and the previous scattered light observables.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.