(Phys.org)--Astronomers have detected a new low-mass eclipsing binary star in an open cluster named NGC 2632, better known as the Beehive Cluster (or Praesepe). The newly identified binary, designated PTFEB132.707+19.810, contains two late-type stars much smaller and less massive than the sun. The new findings were detailed June 28 in a paper published on arXiv.org.
Another bee in the beehive--Astronomers discover binary star in the NGC 2632 cluster
Phys.org - 10 Jul 2017 17:00
(Phys.org)--Astronomers have detected a new low-mass eclipsing binary star in an open cluster named NGC 2632, better known as the Beehive Cluster (or Praesepe). The newly identified binary, designated PTFEB132.707+19.810, contains two late-type stars much smaller and less massive than the sun. The new findings were detailed June 28 in a paper published on arXiv.org.
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