The dusty envelopes of asymptotic giant branch stars with ultraviolet excesses

Open Access

Table 2

Properties of stars for which DUSTY models show no dust component.

Source	T_* (K)	L_* L(L_⊙)
AT Dra	$3400_{- 100}^{+ 100}$ $Mathematical equation: $3400^{+100}_{-100}$$	2500±400
BC CMi	$3400_{- 100}^{+ 100}$ $Mathematical equation: $3400^{+100}_{-100}$$	820±90
BD Cam	$3500_{- 200}^{+ 100}$ $Mathematical equation: $3500^{+100}_{-200}$$	2800±600
BY Boo	$3400_{- 200}^{+ 100}$ $Mathematical equation: $3400^{+100}_{-200}$$	2100±300
CG UMa	$3400_{- 100}^{+ 100}$ $Mathematical equation: $3400^{+100}_{-100}$$	2300±400
DF Leo	$3500_{- 100}^{+ 100}$ $Mathematical equation: $3500^{+100}_{-100}$$	1300±200
ome Vir	$3400_{- 100}^{+ 100}$ $Mathematical equation: $3400^{+100}_{-100}$$	2300±500
RRUMi	$3400_{- 100}^{+ 100}$ $Mathematical equation: $3400^{+100}_{-100}$$	1400±300

Notes. Column 1: name of the source; Column 2: stellar effective temperature; Column 3: bolometric luminosity.

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.