X-ray bursters and dwarf novae - A correspondence

Details X-ray bursters and dwarf novae - A correspondence X-ray bursters and dwarf novae - A correspondence

Nov 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apj...217l.139b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 217, Nov. 1, 1977, p. L139-L141.

Astronomy and Astrophysics

Astrophysics

6

Binary Stars, Neutron Stars, Novae, X Ray Sources, Dwarf Stars, Luminous Intensity, Stellar Mass Ejection, Time Response

Scientific paper

The properties of the X-ray burster MXB 1730-335 are compared directly
with those of the dwarf nova SS Cygni. The striking observational
parallels further support the idea that X-ray bursts are produced by
mass transfer in binary star systems containing a neutron-star member.

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