All Tables
- Table 1:
Methods for determining
/AV ratios.
- Table 2:
Chandra data used in this work.
- Table 3:
X-ray properties of Class III sources in
Oph, IC 348, R CrA, Cha I and Orion Nebula observed with Chandra, and X-ray properties of Class III sources in
Oph observed with XMM-Newton (using the default standard solar ISM abundances in XSPEC). Multiple entries of T correspond to a multiple temperature model.
- Table 4:
Comparison between AJ, and our SED blackbody temperature fitting with those from Luhman & Rieke (1999) for the
Oph sources.
- Table 5:
The
/AV ratios from the
literature (see also Table 1).