OGLE-2002-BLG-360: A dusty anomaly among red nova remnants

Open Access

Table A.1

Table of physical parameters of the stellar remnant and dust shell found from DUSTY modelling.

T_eff (K)	R_⋆ (R_⊙)	r_in (AU)	r_out (pc)	$T_{d}^{i n}$ $\[\mathrm{T}_{d}^{in}\]$ (K)	a_min (μm)	a_max (μm)	q	p
4500	661	208	20	300	0.30	1.00	2	−1.1
Grain type		Composition		Reference
astro-silicates		30%		Draine & Lee (1984)
FeO		10%		Henning et al. (1995)
Al₂O₃		10%		Begemann et al. (1997)
Metallic Fe		25%		Pollack et al. (1994)
				Henning & Stognienko (1996)
Mg_0.9Fe_0.1S		25%		Begemann et al. (1994)

Notes. R_⋆ is the stellar radius, r_in,out is the inner and outer radius of the dust shell, a is the grain size, q is the power law index of the grain size distribution, and p is the power law index of the density distribution.

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.