Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007apj...660l.175b&link_type=abstract
The Astrophysical Journal, Volume 660, Issue 2, pp. L175-L175.
Astronomy and Astrophysics
Astrophysics
1
Scientific paper
In the above-mentioned Letter, we stated that Boss uses a discontinuous internal energy for H2, where H2 contributes 3kT/4mp to the specific internal energy e for T<=100 K and 5kT/4mp for T>100 K, based on his own citations to A. P. Boss (ApJ, 277, 768 [1984]). It was brought to our attention by A. P. Boss (2007, private communication) that he now uses a quadratic interpolation for e between 100 and 200 K (see Fig. 1, left panel). This change is not mentioned in the literature but is alluded to in A. P. Boss (ApJ, 346, 336 [1989]). According to Boss, the interpolation has been used in all his simulations since Boss (1989).
In Figure 1 (right panel), we also illustrate the consequences for Γ1 of Boss's latest e approximation by calculating the specific heat at constant volume cv=de/dT and by relating that to Γ1 (see J. P. Cox & R. T. Giuli, Principles of Stellar Structure [New York: Gordon & Breach, 1968]). This curve is compared with curves for pure para-hydrogen (short-dashed curve), a 3:1 ortho/para-hydrogen mixture (long-dashed curve), where the species are treated as independent, and an equilibrium mixture (solid curve). Because fragmentation becomes more likely as Γ1 is lowered (W. K. M. Rice, G. Lodato, & P. J. Armitage, MNRAS, 364, L56 [2005]), Boss's approximation between 100 and 200 K is likely to make his disks susceptible to fragmentation for that temperature range.
We would like to thank A. P. Boss for his discussions and clarification of his code.
Boley Aaron C.
Durisen Richard H.
Hartquist Thomas W.
Michael Scott
No associations
LandOfFree
Erratum: ``The Internal Energy for Molecular Hydrogen in Gravitationally Unstable Protoplanetary Disks'' (ApJ, 656, L89 [2007]) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Erratum: ``The Internal Energy for Molecular Hydrogen in Gravitationally Unstable Protoplanetary Disks'' (ApJ, 656, L89 [2007]), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Erratum: ``The Internal Energy for Molecular Hydrogen in Gravitationally Unstable Protoplanetary Disks'' (ApJ, 656, L89 [2007]) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1041260