18 Aquilae
{{Short description|Triple star system in the constellation Aquila}}
{{Starbox begin
| name = 18 Aquilae
}}
{{Starbox image
| image=
{{Location mark
|image=Aquila constellation map.svg|alt=|float=center|width=260
|label=|position=right
|mark=Red circle.svg|mark_width=8|mark_link=18 Aql
|x=736|y=274
}}
|caption=Location of 18 Aquilae (circled)
}}
{{Starbox observe
| epoch = J2000
| dec = {{DEC|+11|04|16.4173}}
| appmag_v = 5.072
| constell = Aquila
}}
{{Starbox character
| r-i =
| v-r =
| variable = Eclipsing
}}
{{Starbox astrometry
| parallax = 6.43
| p_error = 0.79
| absmag_v =
}}
{{Starbox orbit
| primary = A
| name = B
| period = 205.16
| eccentricity = 0.23
| inclination = 134.3
| axis = 0.399
}}
{{Starbox orbit
| primary = Aa
| name = Ab
| period_unitless = {{val|1.3023|ul=d}}
| eccentricity =
| inclination =
| axis =
| k1 = 27.6
}}
{{Starbox detail
| component1 = Aa
| radius =
| temperature =
| metal_fe =
| age_myr =
| component2 = Ab
| radius2 =
| temperature2 =
| metal_fe2 =
| rotational_velocity2 =
| age_myr2 =
}}
{{Starbox detail|no_heading=y
| component1 = B
}}
{{Starbox catalog
| names = Y Aquilae, 18 Aql, BD+10 3787, FK5 3525, HD 178125, HIP 93867, HR 7248, SAO 104488
}}
{{Starbox reference
| Simbad = 18+Aql
}}
{{Starbox end}}
18 Aquilae (abbreviated 18 Aql) is a triple star system in the constellation of Aquila. 18 Aquilae is the Flamsteed designation; it also bears the variable star designation Y Aquilae. It has an apparent visual magnitude of 5.07, making it bright enough to be seen with the naked eye. The distance to this system can be estimated from the annual parallax shift of 6.43 mas, yielding a value of around {{Convert|510|ly|pc|abbr=off|lk=on}} away from Earth.
It took decades to determine whether or not 18 Aquilae is a variable star. It was used as a standard star in Benjamin Apthorp Gould's Uranometria Argentina, published in 1879. Gould marked the star with an asterisk, indicating that he thought it is a variable star. Gustav Müller and Paul Kempf noted Gould's opinion in their 1894 work Potsdamer Photometrische Durchmusterung, but stated that their numerous observations did not confirm that the star is variable. That same year, Seth Carlo Chandler reported that 18 Aquilae is a variable star. He stated the star showed an "unmistakable periodicity" and derived a period of 4.986 days - nearly 4 times larger than what the period is now known to be. Chandler gave the star the name Y Aquilae. In 1898, Edward Charles Pickering and Paul S. Yendell announced that their observations of the star "fail to show any evidence of variation". In 1966, Robert Arnold Breinhorst established that Y Aquilae is variable in his PhD thesis.
File:YAqlLightCurve.png for Y Aquilae, plotted from TESS data]]
The inner pair of stars in this system form a spectroscopic binary with a combined magnitude of 5.44 and an orbital period of 1.302 days. The primary component is a giant star with a stellar classification of B8 III. Because the orbital plane is inclined near the line of sight, two form an eclipsing binary system. The eclipse of the primary component causes a 0.04 drop in magnitude, while the eclipse of the secondary results in a decrease of 0.03. At an angular separation of 0.310 arcseconds is the magnitude 6.39 tertiary component. This system has a high peculiar velocity of {{nowrap|29.7 ± 3.9 km/s}} relative to the neighboring stars.
{{clear left}}
References
{{reflist|refs=
{{cite journal | last=Wilson | first=Ralph Elmer | year=1953 | title=General catalogue of stellar radial velocities | journal=Carnegie Institute Washington D.C. Publication | publisher=Carnegie Institution of Washington | bibcode=1953GCRV..C......0W }}
{{Cite journal|last=Tokovinin|first=Andrei|date=2018-03-01|title=The Updated Multiple Star Catalog|journal=The Astrophysical Journal Supplement Series|volume=235|issue=1|pages=6|doi=10.3847/1538-4365/aaa1a5|issn=0067-0049|arxiv=1712.04750|bibcode=2018ApJS..235....6T|s2cid=119047709 |doi-access=free }}
{{cite journal | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E | arxiv = 0806.2878 |date=September 2008| doi-access=free | s2cid=14878976 }}
{{cite simbad | title=18 Aql | access-date=2012-07-25 }}
}}
External links
- [http://aladin.u-strasbg.fr/AladinPreview?-c=19+06+58.6032%2B11+04+16.423&ident=V*+Y+Aql&submit=Aladin+previewer Image 18 Aquilae]
- [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%207248 HR 7248]
{{Stars of Aquila}}
{{DEFAULTSORT:18 Aquilae}}
Category:Aquila (constellation)