New aspects of absorption line formation in intervening turbulent clouds -- II. Monte Carlo simulation of interstellar H+D Ly absorption profiles
Author(s) -
S. A. Levshakov,
W. H. Kegel,
I. E. Mazets
Publication year - 1997
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-8711
pISSN - 0035-8711
DOI - 10.1093/mnras/288.3.802
Subject(s) - physics , monte carlo method , astrophysics , interstellar medium , absorption (acoustics) , line (geometry) , intergalactic travel , line of sight , computational physics , spectral line , interstellar cloud , absorption spectroscopy , molecular cloud , galaxy , astronomy , optics , statistics , stars , redshift , geometry , mathematics
Accelerating Research
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom
Address
John Eccles HouseRobert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom