Statistics – Computation
Scientific paper
Jul 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74..145i&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 1, July 1988, p. 145-160.
Statistics
Computation
31
Cool Stars, Equations Of State, Partitions (Mathematics), Polyatomic Molecules, Stellar Atmospheres, Computational Astrophysics, Least Squares Method, Stellar Composition
Scientific paper
Least square polynomial fits to polyatomic partition functions are presented which are mostly obtained from the revised JANAF thermochemical tables (Chase et al., 1985). The maximum importance of each polyatomic has been calculated based upon equation of state calculations on a grid of temperatures from 1000-6000 K, pressures from 0.1 to 10 to the 6th Pa, M/H abundance ratio values from -2 to 1, and C/O abundance ratio values from 0 to 1. It is noted that the present data, providing the polyatomic information necessary to calculate the equation of state of cool stellar atmospheres, is subject to systematic errors resulting from incomplete spectroscopic information.
No associations
LandOfFree
The partition functions of JANAF polyatomic molecules that significantly affect the stellar atmospheric equation of state 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 The partition functions of JANAF polyatomic molecules that significantly affect the stellar atmospheric equation of state, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The partition functions of JANAF polyatomic molecules that significantly affect the stellar atmospheric equation of state will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1421989