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{{Starbox begin
| name = HD 211575
}}
{{Starbox image
| image = [[File:HD 211575.png|250px]]
| caption= HD 211575 的周邊地區
}}
{{Starbox observe
| epoch = J2000
| constell = [[寶瓶座]]<ref name=Anderson2012/>
| ra = {{RA|22|18|04.2722}}<ref name=Gaia2016/>
| dec = {{DEC|−00|14|15.557}}<ref name=Gaia2016/>
| appmag_v = 6.40<ref name=Paunzen2014/>
}}
{{Starbox character
| type =
| class = F3 V<ref name=Houk1999/>
| b-v = {{Val|0.441|0.003}}<ref name=Anderson2012/>
| variable =
}}
{{Starbox astrometry
| radial_v = {{Val|+14.8|0.5}}<ref name=Casagrande2011/>
| prop_mo_ra = −41.997<ref name=Gaia2016/>
| prop_mo_dec = +54.407<ref name=Gaia2016/>
| parallax = 24.13
| p_error = 0.29
| parallax_footnote = <ref name=vanLeeuwen2007/>
| absmag_v = 3.31<ref name=Paunzen2014/>
}}
{{Starbox detail
| source =
| mass = 1.27<ref name=David2015/>
| radius =
| luminosity = 4.30<ref name=Anderson2012/>
| gravity = 4.15<ref name=Paunzen2014/>
| temperature = {{Val|6574|224|fmt=commas}}<ref name=David2015/>
| metal_fe = {{Val|+0.11|0.11}}<ref name=Casagrande2011/>
| rotational_velocity = 19.0<ref name=Paunzen2014/>
| age_myr = 150<ref name=Casagrande2011/>
}}
{{Starbox catalog
| names = {{odlist | BD=-00°4333 | HD=203222 | HIP=110091 | HR=8507 | SAO=146004 }}<ref name=SIMBAD/>
}}
{{Starbox reference
| Simbad = HD+211575
}}
{{Starbox end}}

'''HD 211575'''位於[[星座]] [[寶瓶座]]，介於[[墳墓二]]（寶瓶座γ）、[[墳墓四]]（寶瓶座π）和[[危宿一]]（寶瓶座α）之間。它是[[大熊座移動星群]]的冠狀體的成員<ref name=Chupina2006/>。

== 參考文獻 ==
<references>
<ref name=SIMBAD>{{cite simbad | title=HD 211575 | access-date=2018-05-11 }}</ref>

<ref name=vanLeeuwen2007>{{citation
| title=Validation of the new Hipparcos reduction
| last1=van Leeuwen | first1=F. | postscript=.
| journal=Astronomy and Astrophysics
| volume=474 | issue=2 | pages=653–664 | year=2007
| arxiv=0708.1752 | bibcode=2007A&A...474..653V
| doi=10.1051/0004-6361:20078357 | s2cid=18759600 }}</ref>

<ref name=Paunzen2014>{{citation
| title=Investigating the possible connection between λ Bootis stars and intermediate Population II type stars
| display-authors=1 | last1=Paunzen | first1=E.
| last2=Iliev | first2=I. Kh. | last3=Fossati | first3=L.
| last4=Heiter | first4=U. | last5=Weiss | first5=W. W.
| journal=Astronomy & Astrophysics
| volume=567 | id=A67 | pages=8 | date=July 2014
| doi=10.1051/0004-6361/201423817 | bibcode=2014A&A...567A..67P
| arxiv=1406.3936 | s2cid=56332289 | postscript=. }}</ref>

<ref name=Gaia2016>{{citation
| title=Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
| last1=Brown | first1=A. G. A. | last2=Vallenari | first2=A.
| last3=Prusti | first3=T. | last4=De Bruijne | first4=J. H. J.
| last5=Mignard | first5=F. | last6=Drimmel | first6=R.
| last7=Babusiaux | first7=C. | last8=Bailer-Jones | first8=C. A. L.
| last9=Bastian | first9=U. | last10=Biermann | first10=M.
| last11=Evans | first11=D. W. | last12=Eyer | first12=L.
| last13=Jansen | first13=F. | last14=Jordi | first14=C.
| last15=Katz | first15=D. | last16=Klioner | first16=S. A.
| last17=Lammers | first17=U. | last18=Lindegren | first18=L.
| last19=Luri | first19=X. | last20=o'Mullane | first20=W.
| last21=Panem | first21=C. | last22=Pourbaix | first22=D.
| last23=Randich | first23=S. | last24=Sartoretti | first24=P.
| last25=Siddiqui | first25=H. I. | last26=Soubiran | first26=C.
| last27=Valette | first27=V. | last28=Van Leeuwen | first28=F.
| last29=Walton | first29=N. A. | last30=Aerts | first30=C.
| display-authors=1 | postscript=.
| journal=Astronomy and Astrophysics
| volume=595 | at=A2 | year=2016
| arxiv=1609.04172 | bibcode=2016A&A...595A...2G
| doi=10.1051/0004-6361/201629512 | s2cid=1828208 }}</ref>

<ref name=David2015>{{citation
| last1=David | first1=Trevor J. | last2=Hillenbrand | first2=Lynne A.
| title=The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets
| journal=The Astrophysical Journal
| volume=804 | issue=2 | pages=146 | year=2015
| bibcode=2015ApJ...804..146D | doi=10.1088/0004-637X/804/2/146
| arxiv=1501.03154 | s2cid=33401607 | postscript=. }}</ref>

<ref name=Casagrande2011>{{citation
| last1=Casagrande | first1=L. | last2=Schönrich | first2=R.
| last3=Asplund | first3=M. | last4=Cassisi | first4=S.
| last5=Ramírez | first5=I. | last6=Meléndez | first6=J.
| last7=Bensby | first7=T. | last8=Feltzing | first8=S.
| title=New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey
| journal=Astronomy & Astrophysics | display-authors=1
| volume=530 | issue=A138 | pages=21 | date=2011
| doi=10.1051/0004-6361/201016276 | bibcode=2011A&A...530A.138C
| arxiv=1103.4651 | s2cid=56118016 | postscript=. }}</ref>

<ref name=Chupina2006>{{citation
| title=Kinematic structure of the corona of the Ursa Major flow found using proper motions and radial velocities of single stars
| display-authors=1 | last1=Chupina | first1=N. V.
| last2=Reva | first2=V. G. | last3=Vereshchagin | first3=S. V.
| journal=Astronomy and Astrophysics | postscript=.
| volume=451 | issue=3 | date=June 2006 | pages=909−916
| doi=10.1051/0004-6361:20054009 | bibcode=2006A&A...451..909C | doi-access=free }}</ref>

<ref name=Houk1999>{{citation
| last1=Houk | first1=N. | last2=Swift | first2=C.
| title=Michigan catalogue of two-dimensional spectral types for the HD Stars
| journal=Michigan Spectral Survey
| volume=5 | year=1999
| bibcode=1999MSS...C05....0H | postscript=. }}</ref>

<ref name=Anderson2012>{{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 | doi=10.1134/S1063773712050015
| arxiv=1108.4971 | s2cid=119257644 | postscript=. }}</ref>
</references>

{{寶瓶座}}

{{DEFAULTSORT:HD 211575}}
[[Category:F型主序星]]
[[Category:寶瓶座]]
[[Category: BD、CD和CP天體]]
[[Category:HD和HDE天體|211575]]
[[Category:HIP天體|110091]]
[[Category:HR天體|8507]]
[[Category:大熊座移動星群]]

HD 211575 - 版本历史

imported>凌雲：​內容擴充

imported>凌雲：內容擴充