HL Aurigae: A pre-contact binary system with a solar-mass companion
Orbital period changes of the near-contact binary (NCB) system, HL Aurigae, are analyzed based upon all the published CCD and photoelectric times of light minimum. It is found that the period of HL Aurigae shows a small-amplitude cyclic oscillation with a period of 6.5 years and an amplitude of 0.d0...
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| Main Authors: | , , |
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| Format: | Journal |
| Published: |
2018
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| Subjects: | |
| Online Access: | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=33645997353&origin=inward http://cmuir.cmu.ac.th/jspui/handle/6653943832/61635 |
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| Institution: | Chiang Mai University |
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