HR Lyrae
Double star HR Lyrae |
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AladinLite | |||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | lyre | ||||||
Right ascension | 18 h 53 m 25.06 s | ||||||
declination | + 29 ° 13 ′ 37.7 ″ | ||||||
Apparent brightness | 15.4 mag | ||||||
Typing | |||||||
rel. Brightness (G-band) |
(15.82 ± 0.01) mag | ||||||
rel. Brightness (J-band) |
(15.06 ± 0.04) mag | ||||||
Variable star type | N / A | ||||||
Astrometry | |||||||
parallax | (0.18 ± 0.03) mas | ||||||
Proper movement | |||||||
Rec. Share: | (−1.93 ± 0.06) mas / a | ||||||
Dec. portion: | (-7.62 ± 0.06) mas / a | ||||||
Physical Properties | |||||||
Other names and catalog entries |
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HR Lyrae also Nova Lyr 1919 was a medium-speed nova of the NA type, which was recorded on December 6, 1919 in the constellation Lyra with an apparent magnitude of 6.5 m by Joanna C. S. Mackie during her systematic search for novas in the Milky Way on photos from Harvard College observatory was discovered.
Depending on the method used, the decrease in brightness was between 31 and 97 days. The amplitude was at least 9.5. Based on the available values, the absolute brightness is set to a maximum of −6.9 m to −7.2 m (± 1.1 m ) and a minimum of +2.3 m to +2.6 m (± 1, 1 m ) estimated.
The star shows an active resting phase with fluctuations in brightness on different time scales. Visual observations over a ten-year period also reveal long periods of time when the star was between 15.4 and 15.7 magnitudes. Some features indicate that it could also be a recurrent nova.
Individual evidence
- ↑ a b c d e f HR Lyr. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed on March 26, 2019 .
- ↑ HR Lyr. In: VSX. AAVSO , accessed March 26, 2019 .
- ^ Bailey, SI: A New Star . In: Popular Astronomy, Vol. 28, 1920, p.134 . 1920. bibcode : 1920PA ..... 28..134B .
- ↑ HR Lyrae (Nova Lyr 1919): from outburst to active quiescence. In: Cornell University. January 25, 2007, accessed March 17, 2019 .