V486 Car is a near-contact binary with component masses 2.1 and 0.4 solar masses, radii 3.2 and 1.48 solar radii, temperatures 10000 K and 6200 K, plus evidence for a ~0.3 solar mass companion at a few AU.
B., 1968b, @doi [ApJ] 10.1086/149712 , https://ui.adsabs.harvard.edu/abs/1968ApJ...153..877L 153, 877
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.SR 2verdicts
UNVERDICTED 2representative citing papers
A derivative-based method estimates mass ratios for overcontact binaries using the time between extrema in the third derivative of light curves, showing agreement with spectroscopic values for most tested systems.
citing papers explorer
-
The Close Binary V486 Carinae
V486 Car is a near-contact binary with component masses 2.1 and 0.4 solar masses, radii 3.2 and 1.48 solar radii, temperatures 10000 K and 6200 K, plus evidence for a ~0.3 solar mass companion at a few AU.
-
Mass ratio estimates for overcontact binaries using the derivatives of light curves
A derivative-based method estimates mass ratios for overcontact binaries using the time between extrema in the third derivative of light curves, showing agreement with spectroscopic values for most tested systems.