Open AccessThe strong 3.3 micron emission line in Wolf-Rayet stars
Author(s) -
P. M. Williams
Publication year - 1982
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/199.1.93
Subject(s) - physics , wolf–rayet star , stars , astrophysics , astronomical spectroscopy , spectral line , emission spectrum , astronomy , line (geometry) , k type main sequence star , stellar classification , t tauri star , 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