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Star in the constellation Aquarius
35 Aquarii is a single
[9]
star located roughly 2,200
light years away from the Sun in the
zodiac
constellation of
Aquarius . 35 Aquarii is its
Flamsteed designation . It is visible to the naked eye as a dim, blue-white hued star with an
apparent visual magnitude of 5.80.
[2] This object is moving closer to the Earth with a heliocentric
radial velocity of −7 km/s,
[2] and is a suspected
runaway star that may have been ejected from an
open cluster as the result of a
binary –binary interaction.
[10]
This is a
blue giant star with a
stellar classification of B2 III;,
[3] a massive star that has
evolved off the
main sequence . It is around 22.5
[4] million years old with a relatively low
projected rotational velocity of 10 km/s.
[7] The star has 10
[4] times the
mass of the Sun and is radiating 1,622
[5] times the
Sun's luminosity from its
photosphere at an
effective temperature of 17,400 K.
[6]
References
^
a
b
c
d
e
Brown, 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 at
VizieR .
^
a
b
c
d
e 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 Houk, Nancy; Smith-Moore, M. (1978), Michigan catalogue of two-dimensional spectral types for the HD stars , vol. 4, Ann Arbor: Dept. of Astronomy, University of Michigan,
Bibcode :
1988mcts.book.....H .
^
a
b
c
d Tetzlaff, 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 .
^
a
b Simón-Díaz, S.; et al. (2017), "The IACOB project. III. New observational clues to understand macroturbulent broadening in massive O- and B-type stars", Astronomy and Astrophysics , 597 : A22,
arXiv :
1608.05508 ,
Bibcode :
2017A&A...597A..22S ,
doi :
10.1051/0004-6361/201628541 ,
S2CID
3478126 .
^
a
b
c Lyubimkov, Leonid S.; et al. (June 2002), "Surface abundances of light elements for a large sample of early B-type stars - II. Basic parameters of 107 stars",
Monthly Notices of the Royal Astronomical Society , 333 (1): 9–26,
Bibcode :
2002MNRAS.333....9L ,
doi :
10.1046/j.1365-8711.2002.05341.x .
^
a
b Strom, Stephen E.; et al. (2005), "B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?", The Astronomical Journal , 129 (2): 809–828,
arXiv :
astro-ph/0410337 ,
Bibcode :
2005AJ....129..809S ,
doi :
10.1086/426748 ,
S2CID
15059129 .
^
"35 Aqr" .
SIMBAD .
Centre de données astronomiques de Strasbourg . Retrieved 2019-05-16 .
^ Eggleton, P. P.; Tokovinin, A. A. (2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society , 389 (2): 869,
arXiv :
0806.2878 ,
Bibcode :
2008MNRAS.389..869E ,
doi :
10.1111/j.1365-2966.2008.13596.x ,
S2CID
14878976 .
^ Leonard, Peter J. T.; Duncan, Martin J. (February 1990), "Runaway Stars from Young Star Clusters Containing Initial Binaries. II. A Mass Spectrum and a Binary Energy Spectrum", Astronomical Journal , 99 : 608,
Bibcode :
1990AJ.....99..608L ,
doi :
10.1086/115354 .