Epsilon Delphini
Star in the constellation Delphinus
Epsilon Delphini (ε Delphini , abbreviated Eps Del , ε Del ), officially named Aldulfin ,[ 12] is a solitary,[ 13] blue-white hued star in the northern constellation of Delphinus . It is visible to the naked eye with an apparent visual magnitude of 4.03.[ 2] Based upon an annual parallax shift of 9.87 mas as seen from the Earth,[ 1] the system is located about 330 light-years from the Sun . At Epsilon Delphini's distance, the visual magnitude is diminished by an extinction factor of 0.11 due to interstellar dust .[ 6] The star is moving closer to the Sun with a radial velocity of −19 km/s.[ 5]
This is a B-type giant star with a stellar classification of B6 III.[ 4] It has 4.6[ 7] times the Sun's radius and is radiating 676[ 8] times the solar luminosity from its photosphere at an effective temperature of 13,614 K.[ 7] The star may be slightly variable, occasionally brightening to magnitude 3.95.[ 3] It is spinning with a projected rotational velocity of 52 km/s.[ 10]
Proper names
ε Delphini (Latinised to Epsilon Delphini ) is the star's Bayer designation .
The star bore the traditional Arabic name ðanab ad-dulfīn or Dzaneb al Delphin, which appeared in the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket and which was translated into Latin as Cauda Delphini , meaning 'the dolphin's tail'.[ 14] In 2016, the IAU organized a Working Group on Star Names (WGSN)[ 15] to catalog and standardize proper names for stars. The WGSN approved the name Aldulfin for this star on 5 September 2017 and it is now so included in the List of IAU-approved Star Names.[ 12]
In Chinese , 敗瓜 (Bài Guā ), meaning Rotten Gourd , refers to an asterism consisting of Epsilon Delphini, Eta Delphini , Theta Delphini , Iota Delphini and Kappa Delphini .[ 16] Consequently, the Chinese name for Epsilon Delphini itself is 敗瓜一 (Bài Guā yī , English: the First Star of Rotten Gourd .).[ 17] From this Chinese name, the name Pae Chaou was formed.[ 18]
References
^ a b c d e f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653– 664, arXiv :0708.1752 , Bibcode :2007A&A...474..653V , doi :10.1051/0004-6361:20078357 , S2CID 18759600 .
^ a b c d Crawford, D. L.; et al. (1971), "Four-color, H-beta, and UBV photometry for bright B-type stars in the northern hemisphere", The Astronomical Journal , 76 : 1058, Bibcode :1971AJ.....76.1058C , doi :10.1086/111220 .
^ a b c Samus, N. N.; et al. (January 2017), "General Catalogue of Variable Stars", Astronomy Reports , GCVS 5.1, 61 (1): 80– 88, Bibcode :2017ARep...61...80S , doi :10.1134/S1063772917010085 , S2CID 125853869 .
^ a b Lesh, Janet Rountree (December 1968), "The Kinematics of the Gould Belt: an Expanding Group?", Astrophysical Journal Supplement , 17 : 371, Bibcode :1968ApJS...17..371L , doi :10.1086/190179 .
^ a b Gontcharov, G. A. (November 2006), "Pulkovo Compilation of Radial Velocities for 35495 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 .
^ a b c Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters , 38 (11): 694– 706, arXiv :1606.09028 , Bibcode :2012AstL...38..694G , doi :10.1134/S1063773712110035 , S2CID 119108982 .
^ a b c d Underhill, A. B.; et al. (November 1979), "Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars", Monthly Notices of the Royal Astronomical Society , 189 (3): 601– 605, Bibcode :1979MNRAS.189..601U , doi :10.1093/mnras/189.3.601 .
^ a b McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society , 427 (1): 343– 57, arXiv :1208.2037 , Bibcode :2012MNRAS.427..343M , doi :10.1111/j.1365-2966.2012.21873.x , S2CID 118665352 .
^ a b Wu, Yue; et al. (January 2011), "Coudé-feed stellar spectral library - atmospheric parameters", Astronomy and Astrophysics , 525 : A71, arXiv :1009.1491 , Bibcode :2011A&A...525A..71W , doi :10.1051/0004-6361/201015014 , S2CID 53480665 .
^ a b Bailey, J. D.; Landstreet, J. D. (2013), "Abundances determined using Si ii and Si iii in B-type stars: Evidence for stratification", Astronomy & Astrophysics , 551 : A30, arXiv :1301.3050 , Bibcode :2013A&A...551A..30B , doi :10.1051/0004-6361/201220671 , S2CID 59291051 .
^ "eps Del -- Variable Star" , SIMBAD Astronomical Database , Centre de Données astronomiques de Strasbourg , retrieved 2017-06-28 .
^ a b "Naming Stars" . IAU.org. Retrieved 16 December 2017 .
^ 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 .
^ Knobel, E. B. (June 1895), "Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket", Monthly Notices of the Royal Astronomical Society , 55 : 429– 438, Bibcode :1895MNRAS..55..429K , doi :10.1093/mnras/55.8.429 .
^ "IAU Working Group on Star Names (WGSN)" . Retrieved 22 May 2016 .
^ (in Chinese) 中國星座神話 , written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7 .
^ (in Chinese) 香港太空館 - 研究資源 - 亮星中英對照表 Archived September 29, 2009, at the Wayback Machine , Hong Kong Space Museum. Accessed on line November 23, 2010.
^ Allen, R. H. (1963), Star Names, Their Lore and Meaning (Dover ed.), p. 201, retrieved 2017-06-29 .