29 Aquarii
{{short description|Binary star in the constellation Aquarius}}
{{Starbox begin
| name = 29 Aquarii
}}
{{Starbox image
| image = 250px
| caption = The light curve of 29 Aquarii, from Hipparcos data
}}
{{Starbox observe
| epoch = J2000
| dec = {{DEC|-16|57|53.3959}}
| constell = Aquarius
}}
{{Starbox character
| class = {{nowrap|A2 V + K0 III}}
| u-b =
| variable =
}}
{{Starbox astrometry
| radial_v = {{Val|+15.0|4.3}}
| parallax = 5.5489
| p_error = 0.1285
| absmag_v =
}}
{{Starbox orbit
| period =
| period_unitless = 0.945 d
| eccentricity = 0.00
| periastron = {{Val|2436814.418|1.0|ul=JD|fmt=commas}}
| k1 = 97.9
}}
{{Starbox catalog
| names = {{odlist | BD=−17°6422 | HD=209278 | HIP=108797 | HR=8396 | SAO=164830 | WDS=J22024-1658 }}
}}
{{Starbox reference
|Simbad=29+Aqr
}}
{{Starbox end}}
29 Aquarii is a binary star system located around 590 light years away from the Sun in the equatorial constellation of Aquarius. 29 Aquarii is the Flamsteed designation; the system also bears the variable star designation DX Aquarii. It is a challenge to view with the naked eye, appearing as a dim star with a combined apparent visual magnitude of 6.39. The system is moving further from the Earth with a heliocentric radial velocity of about +15 km/s.
This is a spectroscopic binary system with a close circular orbit taking just 0.945 days to complete. Despite their proximity, this does not appear to be a contact binary system. The orbital plane of the two stars lies near the line of sight, so they form an Algol-type eclipsing binary. The first component of the system is an A-type main sequence star with a stellar classification of A2 V. Its companion is giant star with a classification of K0 III.
The variability of this system was first noticed in 1965 by W. Strohmeier of Remeis-Observatory in Bamberg, Germany. He later discovered that the variability was caused by a binary companion eclipsing the primary star.
References
{{reflist|refs=
{{cite DR2|6826564991861746688}}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters | postscript=.
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | arxiv=1108.4971
| doi=10.1134/S1063773712050015 | s2cid=119257644 }}
| title=Spectroscopic orbits of the eclipsing binaries DV and CX Aqr
| last1=Paffhausen | first1=W. | last2=Seggewiss | first2=W.
| journal=Astronomy and Astrophysics, Supplemental Series
| volume=24 | pages=29–34 | date=April 1976
| bibcode=1976A&AS...24...29P | postscript=. }}
{{citation | title=BD-17 6422 -- Spectroscopic binary | work=SIMBAD Astronomical Object Database | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=BD-17+6422 | access-date=2012-07-16 | postscript=. }}
| title=The 7.5 Magnitude Limit Sample of Bright Short-Period Binary Stars. I. How Many Contact Binaries Are There?
| last1=Rucinski | first1=Slavek M.
| journal=The Publications of the Astronomical Society of the Pacific
| volume=114 | issue=800 | pages=1124–1142 | date=October 2002
| doi=10.1086/342677 | arxiv=astro-ph/0207144
| bibcode=2002PASP..114.1124R | s2cid=119453008 | postscript=. }}
}}
External links
- [http://aladin.u-strasbg.fr/AladinPreview?-c=V*+DX+Aqr&ident=V*+DX+Aqr&submit=Aladin+previewer Image 29 Aquarii]
{{Stars of Aquarius}}
{{DEFAULTSORT:29 Aquarii}}
Category:A-type main-sequence stars
Category:Spectroscopic binaries
Category:Aquarius (constellation)