New parametrizations of non-Gaussian line-of-sight velocity distribution
Author(s) -
Hongsheng Zhao,
Francisco Prada
Publication year - 1996
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/282.4.1223
Subject(s) - physics , line of sight , gaussian , line (geometry) , distribution (mathematics) , astrophysics , statistical physics , classical mechanics , mathematical analysis , geometry , quantum mechanics , mathematics
A five-parameter fitting formula for the line-of-sight stellar velocitydistributions of steady state systems is proposed. It can faithfully reproducevelocity distributions of theoretical models ranging from nearly Gaussianprofiles to strongly skewed or mildly double-peaked profiles. In contrast tovan der Marel and Franx (1993) and Kuijken and Merrifield (1993), the lineprofiles are required to have neither multi-peaks nor negative velocity wings.Information of the profile is mostly specified by five physically meaningfuland nearly orthogonal fitting parameters.Comment: submitted to MNRAS; 22 pages with 3 tables and 8 figures in uuencoded compressed PS file. Also available at ftp://ibm-1.mpa-garching.mpg.de/pub/hsz/profile.u
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