Figure 2
Balmer-line profiles for HD 191612 at quiescence (, in black) and near emission maximum (φ= 0.89, red); the tickmarks on the y-axis are separated by half the continuum level. The Hα spectrum of HD 209975 is included to demonstrate that a near match to the minimum-state spectrum can be found among normal stars (see Section 3.2 for details). Difference spectra for Hα and Hζ are shown at the bottom of the plot. Velocities are heliocentric.

Balmer-line profiles for HD 191612 at quiescence (formula, in black) and near emission maximum (φ= 0.89, red); the tickmarks on the y-axis are separated by half the continuum level. The Hα spectrum of HD 209975 is included to demonstrate that a near match to the minimum-state spectrum can be found among normal stars (see Section 3.2 for details). Difference spectra for Hα and Hζ are shown at the bottom of the plot. Velocities are heliocentric.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close