Interpreting the line-profile variations of subdwarf B pulsators: the case of PG 1336-018 (NY Virginis)

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Table 1:

Stellar parameters used to model the line-profile variations using the spectral-synthesis codes BRUCE and KYLIE (Townsend 1997).
Parameter	Value
Equatorial rotational velocity (km s^-1)	75
Inclination angle ( $^\circ$ )	80.67
Polar radius ( $R_\odot$ )	0.15
Polar temperature (K)	31 300
Polar gravity (cm s^-2)	5.77
Pulsation period^a (s)	183.98

^a The period detected in our VLT/ UVES data set and in all photometric
campaigns on PG 1336-018 (see Paper I).

Source LaTeX | All tables | In the text

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