Open AccessEnhanced COJ= 2–1/J= 1–0 Ratio as a Marker of Supernova Remnant–Molecular Cloud Interactions: The Cases of W44 and IC 443
Author(s) -
Masumichi Seta,
Tetsuo Hasegawa,
T. M. Dame,
S. Sakamoto,
Tomoharu Oka,
Toshihiro Handa,
Masahiko Hayashi,
JunIchi Morino,
Kazuo Sorai,
K. S. Usuda
Publication year - 1998
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/306141
Subject(s) - physics , astrophysics , supernova remnant , molecular cloud , line (geometry) , line width , supernova , telescope , mean kinetic temperature , astronomy , stars , optics , 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