Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

HD 28375

From Wikipedia, the free encyclopedia
(Redirected from44 Eridani)
Star in the constellation Taurus
HD 28375
Location of HD 28375 (circled)
Observation data
EpochJ2000      EquinoxJ2000
ConstellationTaurus
Right ascension04h 28m 32.12178s[1]
Declination+01° 22′ 50.9687″[1]
Apparent magnitude (V)5.53[2]
Characteristics
Spectral typeB3V[3]
U−Bcolor index-0.55[4]
B−Vcolor index−0.099±0.008[2]
Astrometry
Radial velocity (Rv)18.0±4.3[5] km/s
Proper motion (μ)RA: +19.530[1]mas/yr
Dec.: −20.272[1]mas/yr
Parallax (π)6.8102±0.1690 mas[1]
Distance480 ± 10 ly
(147 ± 4 pc)
Absolute magnitude (MV)0.19[2]
Details
Mass5.0±0.1[6] M
Luminosity126.75[2] L
Surface gravity (log g)4[3] cgs
Temperature13,000[3] K
Metallicity [Fe/H]0.05±0.06[7] dex
Rotational velocity (v sin i)13±3[8] km/s
Age3.1±2.1[6] Myr
Other designations
BD+01°757,FK5 1123,GC 5441,HD 28375,HIP 20884,HR 1415,SAO 111845[9]
Database references
SIMBADdata

HD 28375 is a single[10]star in theequatorialconstellation ofTaurus, near the southern constellation border withEridanus. It was previously known by theFlamsteed designation44 Eridani, although the name has fallen out of use because constellations were redrawn, placing the star out of Eridanus and into Taurus. The star is blue-white in hue and is dimly visible to the naked eye with anapparent visual magnitude of 5.53.[2] The distance to this star is approximately 480 light-years based onparallax.[1] It is drifting further away with aradial velocity of 18 km/s,[5] after having come to within an estimated 249 light-years some 3.7 million years ago.[2]

Cowley (1972) and later Bragança et al. (2012) found astellar classification of B3V[11][12] for this object, matching aB-type main-sequence star. Houk and Swift assigned it a class of B5 III/IV,[13] suggesting it is a moreevolved star that is entering thegiant stage. It has five times themass of the Sun and is around three million years old,[6] with aprojected rotational velocity of just 13 km/s.[8] The star is radiating 127[2] times theluminosity of the Sun from itsphotosphere at aneffective temperature of about 13,000 K.[3]

Aninfrared excess has been detected, indicating the presence of acircumstellar disk. The dust has a temperature of about 119 K and is orbiting67 AU from thestar.[3]

References

[edit]
  1. ^abcdefBrown, A. G. A.; et al. (Gaia collaboration) (August 2018)."Gaia Data Release 2: Summary of the contents and survey properties".Astronomy & Astrophysics.616. A1.arXiv:1804.09365.Bibcode:2018A&A...616A...1G.doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source atVizieR.
  2. ^abcdefgAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  3. ^abcdeLiu, Qiong; Wang, Tinggui; Jiang, Peng (2014). "Bright Debris Disk Candidates Detected with Theakari/far-Infrared Surveyor".The Astronomical Journal.148 (1): 3.arXiv:1308.5593.Bibcode:2014AJ....148....3L.doi:10.1088/0004-6256/148/1/3.S2CID 117353888.
  4. ^Johnson, H. L. (1966). "UBVRIJKL Photometry of the Bright Stars".Communications of the Lunar and Planetary Laboratory.4: 99.Bibcode:1966CoLPL...4...99J.
  5. ^abGontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system".Astronomy Letters.32 (11):759–771.arXiv:1606.08053.Bibcode:2006AstL...32..759G.doi:10.1134/S1063773706110065.S2CID 119231169.
  6. ^abcTetzlaff, N.; et al. (January 2011), "A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun",Monthly Notices of the Royal Astronomical Society,410 (1):190–200,arXiv:1007.4883,Bibcode:2011MNRAS.410..190T,doi:10.1111/j.1365-2966.2010.17434.x,S2CID 118629873
  7. ^Gáspár, András; et al. (2016), "The Correlation between Metallicity and Debris Disk Mass",The Astrophysical Journal,826 (2): 171,arXiv:1604.07403,Bibcode:2016ApJ...826..171G,doi:10.3847/0004-637X/826/2/171,S2CID 119241004.
  8. ^abBragança, G. A.; Daflon, S.; Cunha, K.; Bensby, T.; Oey, M. S.; Walth, G. (2012). "Projected Rotational Velocities and Stellar Characterization of 350 B Stars in the Nearby Galactic Disk".The Astronomical Journal.144 (5): 130.arXiv:1208.1674.Bibcode:2012AJ....144..130B.doi:10.1088/0004-6256/144/5/130.S2CID 118868235.
  9. ^"HD 28375".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-12-18.
  10. ^Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",Monthly Notices of the Royal Astronomical Society,389 (2):869–879,arXiv:0806.2878,Bibcode:2008MNRAS.389..869E,doi:10.1111/j.1365-2966.2008.13596.x,S2CID 14878976.
  11. ^Cowley, A. (November 1972), "Spectral classification of the bright B8 stars",Astronomical Journal,77:750–755,Bibcode:1972AJ.....77..750C,doi:10.1086/111348.
  12. ^Bragança, G. A.; et al. (November 2012), "Projected Rotational Velocities and Stellar Characterization of 350 B Stars in the Nearby Galactic Disk",The Astronomical Journal,144 (5): 10,arXiv:1208.1674,Bibcode:2012AJ....144..130B,doi:10.1088/0004-6256/144/5/130,S2CID 118868235, 130.
  13. ^Houk, N.; Swift, C. (1999), "Michigan catalogue of two-dimensional spectral types for the HD Stars",Michigan Spectral Survey,5,Bibcode:1999MSS...C05....0H
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Nebulae
Astronomical events
Retrieved from "https://en.wikipedia.org/w/index.php?title=HD_28375&oldid=1241784719"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp