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== 参考文献 == {{Reflist|refs= <ref name=GaiaDR2>{{Cite Gaia DR2|2552925644460225152}}</ref> <ref name=Holmberg2009>{{citation | display-authors=1 | last1=Holmberg | first1=J. | last2=Nordström | first2=B. | last3=Andersen | first3=J. | title=The Geneva-Copenhagen survey of the solar neighbourhood. III. Improved distances, ages, and kinematics | volume=501 | issue=3 |date=July 2009 | pages=941–947 | journal=Astronomy and Astrophysics | doi=10.1051/0004-6361/200811191 | bibcode=2009A&A...501..941H | arxiv=0811.3982 | s2cid=118577511 | postscript=. }}</ref> <ref name=aaa521_A12>{{citation | display-authors=1 | last1=Maldonado | first1=J. | last2=Martínez-Arnáiz | first2=R. M. | last3=Eiroa | first3=C. | last4=Montes | first4=D. | last5=Montesinos | first5=B. | title=A spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups | journal=Astronomy and Astrophysics | volume=521 | page=A12 |date=October 2010 | doi=10.1051/0004-6361/201014948 | bibcode=2010A&A...521A..12M |arxiv = 1007.1132 | s2cid=119209183 }}</ref> <ref name="MH08">{{citation | last1=Mamajek | first1=Eric E. | last2=Hillenbrand | first2=Lynne A. | title=Improved Age Estimation for Solar-Type Dwarfs Using Activity-Rotation Diagnostics | journal=The Astrophysical Journal | volume=687 | issue=2 | pages=1264–1293 |date=November 2008 | doi=10.1086/591785 | bibcode=2008ApJ...687.1264M |arxiv = 0807.1686 | s2cid=27151456 }}</ref> <ref name=apj720_2_1290>{{citation | display-authors=1 | last1=Ghezzi | first1=L. | last2=Cunha | first2=K. | last3=Smith | first3=V. V. | last4=de Araújo | first4=F. X. | last5=Schuler | first5=S. C. | last6=de la Reza | first6=R. | title=Stellar Parameters and Metallicities of Stars Hosting Jovian and Neptunian Mass Planets: A Possible Dependence of Planetary Mass on Metallicity | journal=The Astrophysical Journal | volume=720 | issue=2 | pages=1290–1302 |date=September 2010 | doi=10.1088/0004-637X/720/2/1290 | bibcode=2010ApJ...720.1290G |arxiv = 1007.2681 | s2cid=118565025 }}</ref> <ref name="van Belle2009">{{cite journal | title=Directly Determined Linear Radii and Effective Temperatures of Exoplanet Host Stars | url=https://archive.org/details/sim_astrophysical-journal_2009-04-01_694_2/page/1084 | last1=van Belle | first1=Gerard T. | last2=von Braun | first2=Kaspar | journal=The Astrophysical Journal | volume=694 | issue=2 | pages=1085–1098 | date=2009 | arxiv=0901.1206 | bibcode=2009ApJ...694.1085V | doi=10.1088/0004-637X/694/2/1085 | s2cid=18370219 }}</ref> <ref name=aj132_1_161>{{citation | display-authors=1 | last1=Gray | first1=R. O. | last2=Corbally | first2=C. J. | last3=Garrison | first3=R. F. | last4=McFadden | first4=M. T. | last5=Bubar | first5=E. J. | last6=McGahee | first6=C. E. | last7=O'Donoghue | first7=A. A. | last8=Knox | first8=E. R. | title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample | journal=[[The Astronomical Journal]] | volume=132 | issue=1 | pages=161–170 |date=July 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | s2cid=119476992 }}</ref> <ref name=SIMBAD>{{citation | title=HD 4628 -- High proper-motion Star | work=SIMBAD Astronomical Database | publisher=[[Centre de Données astronomiques de Strasbourg]] | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD+4628 | access-date=2016-07-15 | postscript=. | archive-date=2021-11-18 | archive-url=https://web.archive.org/web/20211118152211/http://simbad.u-strasbg.fr/simbad/sim-id?Ident=HD+4628 | dead-url=no }}</ref> <ref name=Mermilliod1986>{{citation | last1=Mermilliod | first1=J.-C. | title=Compilation of Eggen's UBV data, transformed to UBV (unpublished) | journal=Catalogue of Eggen's UBV Data. SIMBAD | date=1986 | bibcode=1986EgUBV........0M | postscript=. }}</ref> }} {{Nearest star systems|5}} {{Stars of Pisces}} {{star-stub}} [[Category:雙魚座]] [[Category:HD和HDE天體|4628]] [[Category:HR天體|0222]] [[Category:SAO天體|109471]]
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