Does the coalescence of white dwarfs produce millisecond pulsars in globular clusters?

Details Does the coalescence of white dwarfs produce millisecond pulsars in globular clusters? Does the coalescence of white dwarfs produce millisecond pulsars in globular clusters?

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apj...411l..75c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 411, no. 2, p. L75-L78.

Astronomy and Astrophysics

Astrophysics

19

Coalescing, Globular Clusters, Pulsars, Stellar Evolution, White Dwarf Stars, Neutron Stars, Supernovae

Scientific paper

Isolated main-sequence stars with initial masses in the range from about 1 to 8 or 9 solar masses will evolve into C + O white dwarfs with masses up to about 1.1 solar mass, and those main-sequence stars with initial masses in the range from about 8 or 9 to 10 or 11 solar masses may produce O + Ne(+Mg) white dwarfs with masses up to about 1.4 solar mass or less. Many such white dwarfs should exist in globular clusters, and pairs of them should coalesce frequently via collisional processes, especially if primordial binaries are present. It is quite possible that most of the short-period millisecond pulsars in the precore-collapse globular clusters have been produced via mergers of white dwarf pairs with total masses exceeding the Chandrasekhar limit.

Affiliated with

Also associated with

No associations

Rating

Does the coalescence of white dwarfs produce millisecond pulsars in globular clusters? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Does the coalescence of white dwarfs produce millisecond pulsars in globular clusters?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Does the coalescence of white dwarfs produce millisecond pulsars in globular clusters? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1069590