NW Puppis

B-type star in the constellation Puppis From Wikipedia, the free encyclopedia

NW Puppis, also known as υ2 Puppis, is a star in the constellation Puppis. Located around 910 light-years distant, it shines with a luminosity approximately 2,000 times that of the Sun and has a surface temperature of 17,930 K.

Right ascension07h 18m 38.18632s[2]
Declination−36° 44 33.8557[2]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
NW Puppis

A light curve for NW Puppis, plotted from TESS data,[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Puppis
Right ascension 07h 18m 38.18632s[2]
Declination −36° 44 33.8557[2]
Apparent magnitude (V) 5.11[3]
Characteristics
Spectral type B3 Vne[4]
Variable type β Cep[3]
Astrometry
Radial velocity (Rv)+18.00±10[5] km/s
Proper motion (μ) RA: −10.848[2] mas/yr
Dec.: +6.699[2] mas/yr
Parallax (π)3.5875±0.1683 mas[2]
Distance910 ± 40 ly
(280 ± 10 pc)
Details
Mass6.5[6] M
Radius5.6[6] R
Luminosity1,995[6] L
Surface gravity (log g)4.07±0.57[7] cgs
Temperature17,930±540[7] K
Rotation1.42 days[8]
Rotational velocity (v sin i)80±8[7] km/s
Age40[6] Myr
Other designations
υ2 Pup, NW Pup, CD−36°3519, HD 57219, HIP 35406, HR 2790, SAO 197837, NW Puppis, υ2 Puppis, Upsilon2 Puppis, Upsilon2 Pup
Database references
SIMBADdata
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The star's variability was first detected in 1970 (based on observations made at La Silla Observatory), and announced by Armand van Hoof in 1973.[9] It was given its variable star designation in 1977.[10] Anamarija Stankov ruled this star out as a Beta Cephei variable,[11] but the GCVS and the International Variable Star Index classify it as both a Beta Cephei variable and a rotating ellipsoidal variable.[12][13] The GCVS lists its period as 0.125 days, but the TESS data shows lower frequency and stochastic brightness variations.[12][14]

Neither component of this double is given a letter in Lacaille's catalogue or the British Association star catalogue.[15][16] Gould gave them the designations (Latin letter) v1 and v2 Puppis, but these are rarely used.[17] Lacaille applied the Greek letter υ to the star now called υ Carinae.[15] The designation υ2 first appeared in several catalogues at the end of the 19th century.[18]

References

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