44 Tauri

Variable star in the constellation Taurus From Wikipedia, the free encyclopedia

44 Tauri, also known as HD 1287 and IM Tauri, is a star located about 210 light years from the Earth, in the constellation Taurus.[3] It is a 5th magnitude star, making it faintly visible to the naked eye of an observer located far from city lights. It is a Delta Scuti variable star, ranging between magnitude 5.37 and 5.58 over a period of about 3.5 hours.[4]

Right ascension04h 10m 49.86084s[3]
Declination+26° 28 51.4365[3]
Apparentmagnitude(V)5.37 - 5.58[4]
Quick facts Constellation, Right ascension ...
44 Tauri

A light curve for IM Tauri, plotted from TESS data.[1] The 3.479 hour period[2] is marked in red.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Taurus
Right ascension 04h 10m 49.86084s[3]
Declination +26° 28 51.4365[3]
Apparent magnitude (V) 5.37 - 5.58[4]
Characteristics
Evolutionary stage main sequence[3][5]
Spectral type F2 IV[6]
Variable type δ Scuti[4]
Astrometry
Radial velocity (Rv)17.43±0.64[3] km/s
Proper motion (μ) RA: −30.919±0.123[3] mas/yr
Dec.: −35.105±0.072[3] mas/yr
Parallax (π)15.4199±0.0863 mas[3]
Distance212 ± 1 ly
(64.9 ± 0.4 pc)
Absolute magnitude (MV)1.44±0.16[7]
Details
Primary
Mass1.89[7] M
Surface gravity (log g)3.6±0.1[6] cgs
Temperature7000±200[8] K
Rotational velocity (v sin i)2±1[8] km/s
Other designations
p Tauri, IM Tauri, BD+26 411, HIP 19513, HD 26322, HR 1287, SAO 76485[9]
Database references
SIMBADdata
Close

In 1966, Ivan Danziger and Robert Dickens discovered that 44 Tauri was a low amplitude variable star, with a period of approximately 3.22 hours.[10] In a follow-up study published the next year, they reported that the period was irregular, indicating beat phenomena, and they classified it as a δ Scuti variable.[11] In 1968, 44 Tauri was given the variable star designation IM Tauri.[12]

44 Tauri has been a popular object for detailed astroseismic and spectroscopic studies, because its very slow (relative to other δ Scuti stars) rotation speed of 3±2 km/sec does not complicate pulsation mode identification or greatly broaden spectral lines.[6][8][13] As of 2010, 44 Tauri had been found to pulsate with 15 independent periods, ranging from 1.89 to 4.52 hours.[6]

References

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