AH Scorpii
{{Short description|Red supergiant star in the constellation Scorpius}}
{{Starbox begin
| name=AH Scorpii
}}
{{Starbox observe
| epoch=J2000
| constell=Scorpius
}}
{{Starbox character
| type=Red supergiant
| u-b=
| variable=SRc{{cite journal|bibcode=2009yCat....102025S|title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}
}}
{{Starbox astrometry
| prop_mo_ra={{val|-2.322|0.115}}
| prop_mo_dec={{val|-2.610|0.068}}
| parallax=0.5632
| p_error=0.0799
| parallax_footnote={{cite Gaia DR3|5979926504430920192}}
| dist_pc={{val|2,260|190|fmt=commas}}
| dist_ly={{val|7,400|620|fmt=commas}}
}}
{{Starbox detail
| luminosity={{val|329000|86000|fmt=commas}}
}}
{{Starbox catalog
| names= AH Sco, AN 223.1907, GSC 07365-00527, HD 155161, HIP 84071, CD−32°12429, 2MASS J17111702-3219308, IRC−30282, IRAS 17080-3215, RAFGL 1927, AAVSO 1704-32
}}
{{Starbox reference
|Simbad=AH+Sco
}}
{{starbox end}}
AH Scorpii (abbreviated to AH Sco) is a red supergiant variable star located in the constellation Scorpius. It is one of the largest stars known by radius and is also one of the most luminous red supergiant stars in the Milky Way.
Distance
Prior to the 21st century, the distance of AH Scorpii was considered to be uncertain, between about 1.5 and {{val|4.6|u=kpc}}. VLBI measurements of the masers have provided an accurate distance of {{val|2,260|u=parsecs|fmt=commas}} based on observation of SiO, H2O, and OH masers in its oxygen-rich circumstellar material. The masers were observed to be approaching the star at 13 km/s, indicating overall contraction at around phase 0.55 of the visual variations.{{cite journal|bibcode=2008ApJ...681.1574C|arxiv=0803.1690|title=VLBI Observations of SiO Masers around AH Scorpii|journal=The Astrophysical Journal|volume=681|issue=2|pages=1574–1583|last1=Chen|first1=Xi|last2=Shen|first2=Zhi-Qiang|year=2008|doi=10.1086/588186|s2cid=7603031}} Gaia Data Release 3 includes a parallax of {{val|0.5632|0.0799|ul=mas}}, corresponding to a distance of about {{val|1.9|u=kpc}}.
Characteristics
File:AHScoLightCurve.png light curve for AH Scorpii, plotted from AAVSO data{{cite web |title=Download Data |url=https://www.aavso.org/data-download |website=aavso.org |publisher=AAVSO |access-date=1 October 2021}}]]
AH Scorpii is a dust-enshrouded red supergiant{{cite journal|bibcode=2005A&A...438..273V|arxiv=astro-ph/0504379|title=An empirical formula for the mass-loss rates of dust-enshrouded red supergiants and oxygen-rich Asymptotic Giant Branch stars|journal=Astronomy and Astrophysics|volume=438|pages=273–289|last1=Van Loon|first1=J. Th.|last2=Cioni|first2=M.-R. L.|last3=Zijlstra|first3=A. A.|last4=Loup|first4=C.|year=2005|issue=1|doi=10.1051/0004-6361:20042555|s2cid=16724272}} and is classified as a semiregular variable star with a main period of 714 days. The total visual magnitude range is 6.5 - 9.6. No long secondary periods have been detected.{{cite journal|bibcode=2009JRASC.103...11P|title=Long Secondary Periods in Pulsating Red Supergiant Stars|journal=Journal of the Royal Astronomical Society of Canada|volume=103|pages=11|last1=Percy|first1=John R.|last2=Sato|first2=Hiromitsu|year=2009|issue=1}} Modelling of AH Scorpii near maximum light has determined an effective temperature of {{val|3,682|190|fmt=commas|u=K}} and a luminosity of {{val|330,000|86,000|fmt=commas|u={{solar luminosity}}}}. A radius of {{solar radius|{{val|1,411|124|fmt=commas}}}} was determined from an angular diameter of {{val|5.81|0.15|ul=mas}} and the given distance of {{val|2.26|0.19|u=kpc}}. Its angular diameter was re-measured at {{Val|5.05|0.5|u=mas}} in 2023.{{Cite journal |last1=González-Torà |first1=G. |last2=Wittkowski |first2=M. |last3=Davies |first3=B. |last4=Plez |first4=B. |date=December 19, 2023 |title=The effect of winds on atmospheric layers of red supergiants II. Modelling VLTI/GRAVITY and MATISSE observations of AH Sco, KW Sgr, V602 Car, CK Car and V460 Car |journal=Astronomy & Astrophysics |volume=683 |pages=A19 |doi=10.1051/0004-6361/202348047 |issn=0004-6361|arxiv=2312.12521 |bibcode=2024A&A...683A..19G }}
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