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词条 HD 211073
释义

  1. References

{{Starbox begin
| name = HD 211073
}}{{Starbox observe
| epoch = J2000.0
| constell = Lacerta
| ra = {{RA|22|13|52.72731}}[1]
| dec = {{DEC|+39|42|53.7442}}[1]
| appmag_v = 4.50[3] (4.49–4.55)[4]
}}{{Starbox character
| class = K2.5 III[5]
| b-v = 1.39[6]
| u-b =
| variable =
}}{{Starbox astrometry
| radial_v = {{Val|−11.69|0.13}}[6]
| prop_mo_ra = +39.155[1]
| prop_mo_dec = +18.441[1]
| parallax = 5.5806
| p_error = 0.2705
| parallax_footnote = [1]
| absmag_v = −1.34[3]
}}{{Starbox detail
| source = [12]
| component1 = HD 211073 Aa
| mass = {{Val|2.23|0.22|0.26}}
| radius = {{Val|45.69|2.17|2.39}}
| luminosity = {{Val|573.50|51.88|61.58}}
| temperature = {{Val|4180|12|14|fmt=commas}}
| gravity = {{Val|1.46|0.05|0.04}}
| rotational_velocity = {{Val|2.9|1.0}}[6]
| metal_fe =
| age_myr = {{Val|1.00|0.38|0.19}}
}}{{Starbox catalog
| names = {{odlist | BD=+38° 4711 | FK5=1583 | HD=211073 | HIP=109754 | HR=8485 | SAO=72155 | WDS=J22139+3943 | NSV=14076 }}
}}{{Starbox reference
| Simbad = HD+211073
}}{{Starbox end}}HD 211073 is a triple star[15] system in the northern constellation Lacerta, located around 580[1] light years from the Sun. It is visible to the naked eye as a faint orange-hued star with a baseline apparent visual magnitude of 4.50.[3] The system is moving closer to the Earth with a heliocentric radial velocity of −11.7 km/s.[6]

The primary member, designated component Aa, is an evolved giant star with a stellar classification of K2.5 III[5] that is most likely (98% chance) on the horizontal branch.[12] It is a suspected variable star that ranges in magnitude from 4.49 down to 4.55.[4] This star is around a billion years old with 2.2 times the mass of the Sun and has expanded to 46 times the Sun's radius. It is radiating about 574 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,180 K.[12]

As of 2005, the inner pair of stars (Aa + Ab) in this system had an angular separation of {{Val|0.20|ul=arcsecond}} along a position angle (PA) of 170°. The magnitude 8.15 component Ac was separated from Aa by {{Val|0.30|u=arcsecond}} with a PA of 27°, as of 2010. As of 2015, the magnitude 10.60 visual companion, designated component B, was separated from the primary by {{val|30.50|u=arcsecond}} along a PA of 190°.[23]

References

1. ^{{cite DR2|1955662200880678272}}
2. ^{{citation | title=XHIP: An extended hipparcos compilation | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | bibcode=2012AstL...38..331A | arxiv=1108.4971 | doi=10.1134/S1063773712050015 | postscript=. }}
3. ^{{citation | display-authors=1 | last1=Mason | first1=Brian D. | last2=Wycoff | first2=Gary L. | last3=Hartkopf | first3=William I. | last4=Douglass | first4=Geoffrey G. | last5=Worley | first5=Charles E. | title=The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog | journal=The Astronomical Journal | postscript=. | volume=122 | issue=6 | pages=3466–3471 | date=December 2001 | doi=10.1086/323920 | bibcode=2001AJ....122.3466M }}
4. ^{{citation | title=General Catalogue of Variable Stars | display-authors=1 | last1=Samus | first1=N. N. | last2=Kazarovets | first2=E. V. | last3=Durlevich | first3=O. V. | last4=Kireeva | first4=N. N. | last5=Pastukhova | first5=E. N. | version=5.1 | journal=Astronomy Reports | year=2017 | volume=61 | issue=1 | pages=80–88 | bibcode=2017ARep...61...80S | postscript=. }}
5. ^{{citation | last1=De Medeiros | first1=J. R. | last2=Mayor | first2=M. | title=A catalog of rotational and radial velocities for evolved stars | journal=Astronomy and Astrophysics Supplement Series | volume=139 | issue=3 | pages=433 | year=1999 | bibcode=1999A&AS..139..433D | postscript=. | doi=10.1051/aas:1999401 | arxiv=astro-ph/0608248 }}
6. ^{{citation | last1=Keenan | first1=Philip C. | last2=McNeil | first2=Raymond C. | title=The Perkins catalog of revised MK types for the cooler stars | journal=Astrophysical Journal Supplement Series | volume=71 | pages=245 | year=1989 | postscript=. | bibcode=1989ApJS...71..245K | doi=10.1086/191373 }}
7. ^{{citation | 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 | date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | postscript=. | bibcode=2008MNRAS.389..869E | arxiv=0806.2878 }}
8. ^{{citation | title=Precise radial velocities of giant stars. X. Bayesian stellar parameters and evolutionary stages for 372 giant stars from the Lick planet search | display-authors=1 | last1=Stock | first1=Stephan | last2=Reffert | first2=Sabine | last3=Quirrenbach | first3=Andreas | journal=Astronomy & Astrophysics | volume=616 | id=A33 | pages=15 | date=August 2018 | doi=10.1051/0004-6361/201833111 | arxiv=1805.04094 | bibcode=2018A&A...616A..33S | postscript=. }}
[1][2][3][4][5][6][7][8]
}}{{Stars of Lacerta}}

9 : K-type giants|Horizontal-branch stars|Suspected variables|Triple star systems|Lacerta (constellation)|Durchmusterung objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects

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