| Issue |
A&A
Volume 416, Number 1, March II 2004
|
|
|---|---|---|
| Page(s) | 187 - 190 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361:20031746 | |
| Published online | 26 February 2004 | |
The heat capacity of water ice in interstellar or interplanetary conditions
Isaac Newton Institute Kiev Branch, Main Astronomical Observatory of the National Academy of Sciences of Ukraine (MAO NASU), Golosiiv, 03680, Kyiv-22, Ukraine
Corresponding author: shulman@mao.kiev.ua
Received:
12
November
2002
Accepted:
24
November
2003
Three empirical equations are proposed to describe the existing
experimental data on the heat capacity of water ice for 
. This may be important for the rate
of non-stationary thermal processes at very low temperatures in cometary
nuclei or cosmogonical scenarios.
Key words: ISM: molecules / comets: general / stars: formation
© ESO, 2004
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.