Interior structura variations in the secondary components of two algol-type eclipsing binary systems: SW Cygni and RR Draconis
SW Cyg and DD Dra are two Algol-type eclipsing binary systems. Both contain an A2-type main-sequence primary and a K0-type secondary component with a rather deep primary light minimum in their light curves (2.m6 and 3.m 8, respectively). In the present paper, orbital period changes of these stars ar...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
2014
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| Online Access: | http://www.scopus.com/inward/record.url?eid=2-s2.0-0036901867&partnerID=40&md5=344ad865ec944f690f188c38c93a6776 http://cmuir.cmu.ac.th/handle/6653943832/5182 |
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| Institution: | Chiang Mai University |
| Language: | English |
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