From Wikipedia, the free encyclopedia
Binary star system in the constellation Corona Borealis
Iota Coronae Borealis ,
Latinized from ι Coronae Borealis , is a
binary star
[6] system in the
constellation
Corona Borealis . It is visible to the naked eye with a combined
apparent visual magnitude of is 4.96.
[2] Based upon an annual
parallax shift of 10.46
mas as seen from the Earth,
[1] it is located about 312
light years from the
Sun .
This is a single-lined
spectroscopic binary with an
orbital period of 35.5 days and an
eccentricity of 0.56.
[6] The visible member, component A, has a
stellar classification of A0 IIIp(HgMnEu)s ,
[3] indicating it is a
chemically peculiar
mercury-manganese star with narrow
absorption lines . The secondary member, component B, appears to be an
A-type star .
[11]
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 Fernie, J. D. (1983), "New UBVRI photometry for 900 supergiants", Astrophysical Journal Supplement Series , 52 : 7,
Bibcode :
1983ApJS...52....7F ,
doi :
10.1086/190856 .
^
a
b Abt, Helmut A.; Morrell, Nidia I. (1995), "The Relation between Rotational Velocities and Spectral Peculiarities among A-Type Stars", Astrophysical Journal Supplement , 99 : 135,
Bibcode :
1995ApJS...99..135A ,
doi :
10.1086/192182 .
^ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics , 546 : 14,
arXiv :
1208.3048 ,
Bibcode :
2012A&A...546A..61D ,
doi :
10.1051/0004-6361/201219219 ,
S2CID
59451347 , A61.
^ Anderson, 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 .
^
a
b
c Pourbaix, D.; et al. (2004), "SB9: The ninth catalogue of spectroscopic binary orbits",
Astronomy and Astrophysics , 424 (2): 727–732,
arXiv :
astro-ph/0406573 ,
Bibcode :
2004A&A...424..727P ,
doi :
10.1051/0004-6361:20041213 ,
S2CID
119387088 .
^ 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
c Prugniel, Ph.; Vauglin, I.; Koleva, M. (July 2011), "The atmospheric parameters and spectral interpolator for the MILES stars", Astronomy & Astrophysics , 531 : A165,
arXiv :
1104.4952 ,
Bibcode :
2011A&A...531A.165P ,
doi :
10.1051/0004-6361/201116769 ,
S2CID
54940439 .
^ Royer, F.; et al. (October 2002), "Rotational velocities of A-type stars in the northern hemisphere. II. Measurement of v sin i", Astronomy and Astrophysics , 393 : 897–911,
arXiv :
astro-ph/0205255 ,
Bibcode :
2002A&A...393..897R ,
doi :
10.1051/0004-6361:20020943 ,
S2CID
14070763 .
^
"iot CrB" ,
SIMBAD ,
Centre de données astronomiques de Strasbourg , retrieved 2017-05-05 .
^ Dubaj, D.; Monier, R.; Alecian, G.; Leblanc, F. (December 2005),
Casoli, F. ; Contini, T.; Hameury, J.M.; Pagani, L. (eds.), "Abundance determinations for the two components of the spectroscopic binary star HD143807", SF2A-2005: Semaine de l'Astrophysique Française , EdP-Sciences: 335,
Bibcode :
2005sf2a.conf..335D .