{'fraction_non_alphanumeric': 0.015151515151515152, 'fraction_numerical': 0.0, 'mean_word_length': 4.613207547169812, 'pattern_counts': {'":': 0, '<': 0, '<?xml version=': 0, '>': 0, 'https://': 0, 'lorem ipsum': 0, 'www.': 0, 'xml': 0}, 'pii_count': 0, 'substrings_counts': 0, 'word_list_counts': {'cursed_substrings.json': 0, 'profanity_word_list.json': 0, 'sexual_word_list.json': 0, 'zh_pornsignals.json': 0}}
Pressure at the ISM-halo interface: A reheating frequency dependence

The dependence of the thermal pressure of hot galactic halos on a model 
 parameter describing the frequency of major reheating episodes during 
 galactic history is investigated. Pressure on the interface between 
 interstellar medium and the halo gas is especially interesting, since 
 empirical evidence here offers one of the simplest constraints on halo 
 models. It is shown that two-phase model of Mo & Miralda-Escude is 
 sufficiently robust with respect to uncertainties in the average interval 
 between reheating.