Pulsating B-Type Stars In The Young Open Cluster H Persei (Ngc 869)

PROCEEDINGS OF THE SECOND HELAS INTERNATIONAL CONFERENCE: HELIOSEISMOLOGY, ASTEROSEISMOLOGY AND MHD CONNECTIONS(2008)

Cited 3|Views4
No score
Abstract
We announce the discovery of six beta Cephei stars and many other variable stars in the young open cluster h Persei (NGC 869). The cluster seems to be very rich in variable B-type stars, similarly to its twin, chi Persei (NGC 884).
More
Translated text
Key words
variable stars,open clusters
AI Read Science
Must-Reading Tree
Example
Generate MRT to find the research sequence of this paper
Chat Paper
Summary is being generated by the instructions you defined