Further Evidence of a Brown Dwarf Orbiting the Post-Common Envelope Eclipsing Binary V470 Cam (HS 0705+6700)
Several post-common envelope binaries have slightly increasing, decreasing or oscillating orbital periods. One of several possible explanations is light travel-time changes, caused by the binary centre-of-mass being perturbed by the gravitational pull of a third body. Further studies are necessary b...
Main Authors: | Bogensberger David, Clarke Fraser, Lynas-Gray Anthony Eugene |
---|---|
Format: | Article |
Language: | English |
Published: |
De Gruyter
2017-12-01
|
Series: | Open Astronomy |
Subjects: | |
Online Access: | https://doi.org/10.1515/astro-2017-0015 |
Similar Items
-
Further evidence of a brown dwarf orbiting the post-common envelope eclipsing binary V470 cam (HS 0705+6700)
by: Bogensberger, D, et al.
Published: (2017) -
Observations of Two Unusual Eclipsing Binaries, FN Cam and AG Vir
by: Avvakumova E. A., et al.
Published: (2014-12-01) -
Physical Parameters of 11,100 Short-period ASAS-SN Eclipsing Contact Binaries
by: Xu-Zhi Li, et al.
Published: (2024-01-01) -
Multifilter Time-series Observations of Eleven Blue Short-period ATLAS Variable Stars
by: C. Koen, et al.
Published: (2023-01-01) -
The Evolutionary Statuses of Solar Type Detached Eclipsing Binary Stars
by: Chanisa Kanjanascul, et al.
Published: (2012-06-01)