Astronomy 162: White Dwarfs and Novae
Edit Page
Report
Scan day: 09 February 2014 UTC
29
Virus safety - good
Description: Short on text, but contains excellent images, diagrams and a table of the brightest white dwarfs
Subrahmanyan Chandrasekhar predicted while a very young man in the 1930s that there was a limiting mass for white dwarf stars: no white dwarf could be stable against gravitational collapse if it exceeded this mass, which is about 1.4-1.5 solar masses, depending on the detailed composition of the white dwarf. The idea was not very well received by many established astronomers, who considered it absurd that a white dwarf could have a limiting mass. Much later, Chandrasekhar's brilliant idea was completely accepted within the astrophysics community and he eventually won a Nobel Prize for his deep theoretical contributions to astrophysics. Today, all textbooks on stars describe the Chandrasekhar Limiting Mass for white dwarfs as central to the structure of white dwarfs
Size: 780 chars
Contact Information
Email: —
Phone&Fax: —
Address: —
Extended: —
WEBSITE Info
Page title: | White Dwarfs and Novae |
Keywords: | |
Description: | |
IP-address: | 160.36.28.37 |
WHOIS Info
NS | Name Servers: NS0.UTK.EDU 160.36.0.66 NS1.UTK.EDU 160.36.128.66 |
WHOIS | |
Date | activated: 04-Jun-1987 last updated: 31-Mar-2011 expires: 31-Jul-2014 |