Supersonic Line Broadening within Young and Massive Super Star Clusters

Number of the records: 1

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SYSNO ASEP	0355286
Document Type	J - Journal Article
R&D Document Type	Journal Article
Subsidiary J	Článek ve WOS
Title	Supersonic Line Broadening within Young and Massive Super Star Clusters
Author(s)	Tenorio-Tagle, G. (ES) Wünsch, Richard (ASU-R)_{RID, ORCID} Silich, S. (MX) Munoz-Tunon, C. (ES) Palouš, Jan (ASU-R)_{RID, ORCID}
Source Title	Astrophysical Journal - ISSN 0004-637X Roč. 708, č. 2 (2010), s. 1621-1627
Number of pages	7 s.
Language	eng - English
Country	US - United States
Keywords	galaxies ; star clusters ; H II regions
Subject RIV	BN - Astronomy, Celestial Mechanics, Astrophysics
R&D Projects	LC06014 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
CEZ	AV0Z10030501 - ASU-R (2005-2011)
UT WOS	000273021000057
DOI	10.1088/0004-637X/708/2/1621
Annotation	The origin of supersonic infrared and radio recombination nebular lines often detected in young and massive superstar clusters is discussed.
Workplace	Astronomical Institute
Contact	Radka Svašková, bibl@asu.cas.cz, Tel.: 323 620 326
Year of Publishing	2011

Number of the records: 1