Fig. 4.
Ratios of the EQWs of the Ca ii IRT emission lines. The circle symbols represent the PMS stars in the molecular clouds and moving groups. The PMS stars are separated into two groups by the median of their FWHMλ8542; the open circles show the group of PMS stars with a broader FWHMλ8542 than the median. The filled circles represent the narrower group. The low-mass stars in the young open clusters IC 2391 and IC 2602 are plotted as cross symbols (Marsden et al. 2009). The dotted line represents isothermal slabs (T = 5000 K) in LTE (Herbig & Soderblom 1980; Hamann & Persson 1992). The black star symbols on the line correspond to slab optical depths of 10, 100, and 1000, beginning from the upper right. The arrow in the lower right is the redding vector with AV = 10 mag.

Ratios of the EQWs of the Ca ii IRT emission lines. The circle symbols represent the PMS stars in the molecular clouds and moving groups. The PMS stars are separated into two groups by the median of their FWHMλ8542; the open circles show the group of PMS stars with a broader FWHMλ8542 than the median. The filled circles represent the narrower group. The low-mass stars in the young open clusters IC 2391 and IC 2602 are plotted as cross symbols (Marsden et al. 2009). The dotted line represents isothermal slabs (T = 5000 K) in LTE (Herbig & Soderblom 1980; Hamann & Persson 1992). The black star symbols on the line correspond to slab optical depths of 10, 100, and 1000, beginning from the upper right. The arrow in the lower right is the redding vector with AV = 10 mag.

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