HD 28843

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HD 28843
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Eridanus
Right ascension 04h 32m 37.55373s[1]
Declination −03° 12′ 34.3448″[1]
Apparent magnitude (V) 5.70 - 5.84[2]
Characteristics
Spectral type B9III[3]
U−B color index −0.55[4]
B−V color index −0.14[4]
Variable type SX Arietis[5]
Astrometry
Radial velocity (Rv)18±7[3] km/s
Proper motion (μ) RA: 18.227±0.068[1] mas/yr
Dec.: −16.177±0.054[1] mas/yr
Parallax (π)5.8958±0.0608 mas[1]
Distance553 ± 6 ly
(170 ± 2 pc)
Absolute magnitude (MV)−0.7[6]
Details
Mass4.20±0.6[7] M
Radius3.4[1] R
Luminosity324+57
−48
[7] L
Surface gravity (log g)3.86[1] cgs
Temperature14800±200[7] K
Metallicity [Fe/H]−0.166[8] dex
Rotation1.37381±0.00001 d[9]
Rotational velocity (v sin i)91[7] km/s
Other designations
DZ Eri, HR 1441, HIP 21192, SAO 131279[10]
Database references
SIMBADdata
File:DZEriLightCurve.png
A light curve for DZ Eridani, plotted from TESS data[11]

HD 28843, also known as HR 1441 and DZ Eridani, is a star about 550 light years from the Earth, in the constellation Eridanus.[1] It is a 5th magnitude star, so it will be faintly visible to the naked eye of an observer far from city lights. It is a variable star, whose brightness varies slightly from 5.70 to 5.84 during its 1.374 day rotation period.[2][9] It is a member of the μ Tauri Association, a group of young stars within the larger Cassiopeia-Taurus Structure.[3]

In 1969 Mercedes Jaschek et al. determined that HD 28843 is a helium-weak star, based on its B-V color index being bluer (more negative) than would be expected for a star with its spectral type.[12] In 1977, Robert Davis reported that the star has an overabundance of silicon.[13] It is classified as a chemically peculiar star.[14]

Henning Jorgensen et al. reported that HD 28843 was a "suspected variable star" in 1971.[15] The variability of the star was firmly established in 1977 by Holger Pedersen and Bjarne Thomsen, during a spectroscopic and photometric study of helium weak and helium strong stars. They determined its period to be 1.374±0.006 days.[16] In 1978 the star was given the variable star designation DZ Eridani.[17]

Ermanno Borra et al. reported in 1983 the detection of the magnetic field of HD 28843, and estimated its strength to be a few hundred gauss.[18] Later data from the International Ultraviolet Explorer implied a field strength of 250 gauss.[19]

M. Farthmann et al. reported in 1994 that high spectral resolution observations of the 4471Å spectral line of neutral helium can be explained if HD 28843 has two helium-enriched circular "caps" separated by a region with a dramatically lower helium abundance.[20]

References

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  1. ^ a b c d e f g h Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). Gaia DR3 record for this source at VizieR.
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  20. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).