☆
4.7
Article
Star formation rates in cooling flow clusters:: A UV pilot study with archival XMM-Newton optical monitor data
ASTROPHYSICAL JOURNAL (2005)
Rate this paper
The primary rating indicates the level of overall quality for the paper. Secondary ratings independently reflect strengths or weaknesses of the paper.
Find Funding. Review Successful Grants.
Explore over 25,000 new funding opportunities and over 6,000,000 successful grants.
ExploreAsk a Question. Answer a Question.
Quickly pose questions to the entire community. Debate answers and get clarity on the most important issues facing researchers.
Get Started