Talk:V803 Centauri

This article is rated Stub-class on Wikipedia's content assessment scale.
It is of interest to the following WikiProjects:

Astronomy: Astronomical objects Low‑importance

	Astronomy portal This article is within the scope of WikiProject Astronomy, which collaborates on articles related to Astronomy on Wikipedia.AstronomyWikipedia:WikiProject AstronomyTemplate:WikiProject AstronomyAstronomy articles
Low	This article has been rated as Low-importance on the project's importance scale.
	This article is supported by WikiProject Astronomical objects, which collaborates on articles related to astronomical objects.
	An appropriate image needs to be added to this article, or the current one needs to be updated. Once this has been done, please remove the `\|needs-image=yes` parameter from this template.

What period(s) have been measured/reported ?[edit]

What period(s) have been measured/reported ? - If none, can we infer we're nearly face on to the orbits ? - Rod57 (talk) 12:50, 23 July 2019 (UTC)[reply]

The orbital period is 27 minutes. This is a stub article, and should be expanded with information such as this, supported by reliable references. Although the orbit is not reliably determined, the inclination is thought to be fairly low.^[1] Lithopsian (talk) 13:29, 23 July 2019 (UTC)[reply]

References

^ Roelofs, G. H. A.; Groot, P. J.; Nelemans, G.; Marsh, T. R.; Steeghs, D. (2007). "On the orbital periods of the AM CVN stars HP Librae and V803 Centauri". Monthly Notices of the Royal Astronomical Society. 379 (1): 176–182. arXiv:0705.0402. Bibcode:2007MNRAS.379..176R. doi:10.1111/j.1365-2966.2007.11931.x.

[1] Roelofs, G. H. A.; Groot, P. J.; Nelemans, G.; Marsh, T. R.; Steeghs, D. (2007). "On the orbital periods of the AM CVN stars HP Librae and V803 Centauri". Monthly Notices of the Royal Astronomical Society. 379 (1): 176–182. arXiv:0705.0402. Bibcode:2007MNRAS.379..176R. doi:10.1111/j.1365-2966.2007.11931.x.

[1]