Y Lyncis

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Y Lyncis

A visual band light curve for Y Lyncis, adapted from Percy et al. (2001).[1] The top panel shows the brightness variation over a period of several years, and the lower panel shows shorter time scale variations.
Observation data
Epoch J2000      Equinox J2000
Constellation Lynx
Right ascension 07h 28m 11.61657s[2]
Declination +45° 59′ 26.2295″[2]
Apparent magnitude (V) 6.2 - 8.9[3]
Characteristics
Spectral type M6S Ib[4]
Variable type
SRc[4]
Distance
1,160 ± 50 ly
(360 ± 10 pc)
Details
dex
SAO
 41784
Database references
SIMBADdata

Y Lyncis is a

semiregular variable star in the constellation Lynx. It is an asymptotic giant branch
star of spectral type M6S, with a luminosity class of Ib, indicating a supergiant luminosity. It is around 1,160 light years away.

Y Lyncis ranges in brightness from magnitude 6.2 to 8.9. Its changes in brightness are complex with at least two different periods showing. The

long secondary period with an amplitude of 0.2 magnitudes and duration 1,300 days. The long secondary period variations are possibly caused by long-lived convection cells.[9]

Y Lyncis has a mass around 1.5-2.0 M and a luminosity around 10,000 L. It is a thermally pulsing

asymptotic giant branch star, an evolved star with a carbon-oxygen core that is fusing helium in a shell and hydrogen in a separate shell.[10] It is also an S-type star, where third dredge-ups have brought some carbon to the surface, but not enough to create a carbon star.[6]

References