The Solar Neighborhood XLIV: RECONS Discoveries within 10 parsecs

被引:87
作者
Henry, Todd J. [1 ]
Jao, Wei-Chun [2 ]
Winters, Jennifer G. [3 ]
Dieterich, Sergio B. [4 ]
Finch, Charlie T. [5 ]
Ianna, Philip A. [1 ]
Riedel, Adric R. [6 ]
Silverstein, Michele L. [2 ]
Subasavage, John P. [7 ]
Vrijmoet, Eliot Halley [2 ]
机构
[1] RECONS Inst, Chambersburg, PA 17201 USA
[2] Georgia State Univ, Dept Phys & Astron, Atlanta, GA 30302 USA
[3] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[4] Carnegie Inst Sci, Dept Terr Magnetism, 5241 Broad Branch Rd NW, Washington, DC 20015 USA
[5] US Naval Observ, Astrometry Dept, Washington, DC 20392 USA
[6] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[7] US Naval Observ, Flagstaff, AZ 86001 USA
基金
美国国家科学基金会; 英国科学技术设施理事会;
关键词
astrometry; solar neighborhood; stars: distances; stars: low-mass; stars: statistics; surveys; PROPER MOTION STARS; 0.9 M PROGRAM; M TELESCOPE PROGRAM; WHITE-DWARF SAMPLE; GUIDANCE SENSOR 3; LOW-MASS STARS; NEARBY STARS; SPECTROSCOPIC SURVEY; PROXIMA CENTAURI; BROWN DWARF;
D O I
10.3847/1538-3881/aac262
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We describe the 44 systems discovered to be within 10 pc of the Sun by the RECONS team, primarily via the long-term astrometry program at the CTIO/SMARTS 0.9 m that began in 1999. The systems-including 41 with red dwarf primaries, 2 white dwarfs, and 1 brown dwarf-have trigonometric parallaxes greater than 100 mas, with errors of 0.4-2.4 mas in all but one case. We provide updated astrometric, photometric (VRIJHK magnitudes), spectral type, and multiplicity information here. Among these are 14 systems that are new entries to the 10 pc sample, including the first parallaxes for 9 systems and new values for 5 systems that had previous parallaxes with errors greater than 10 mas or values placing them beyond 10 pc. We also provide new data for 22 systems known to lie within 10 pc and 9 systems reported to be closer than that horizon but for which new parallaxes place them further away, bringing the total to 75 systems. The 44 systems added by RECONS comprise one of every 7 systems known within 10 pc. We illustrate the evolution of the 10 pc sample from the 191 systems known when the final Yale Parallax Catalog was published in 1995 to the 317 systems known today. Even so close to the Sun, additional discoveries of white, red, and brown dwarfs are possible, both as primaries and secondaries, although we estimate that at least 90% of the stellar systems closer than 10 pc have now been identified.
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页数:23
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共 112 条
  • [1] PARALLAXES OF SOUTHERN EXTREMELY COOL OBJECTS. I. TARGETS, PROPER MOTIONS, AND FIRST RESULTS
    Andrei, A. H.
    Smart, R. L.
    Penna, J. L.
    d'Avila, V. A.
    Bucciarelli, B.
    Camargo, J. I. B.
    Crosta, M. T.
    Dapra, M.
    Goldman, B.
    Jones, H. R. A.
    Lattanzi, M. G.
    Nicastro, L.
    Pinfield, D. J.
    da Silva Neto, D. N.
    Teixeira, R.
    [J]. ASTRONOMICAL JOURNAL, 2011, 141 (02)
  • [2] The Solar Neighborhood. XXXX. Parallax Results from the CTIOPI 0.9 m Program: New Young Stars Near the Sun
    Bartlett, Jennifer L.
    Lurie, John C.
    Riedel, Adric
    Ianna, Philip A.
    Jao, Wei-Chun
    Henry, Todd J.
    Winters, Jennifer G.
    Finch, Charlie T.
    Subasavage, John P.
    [J]. ASTRONOMICAL JOURNAL, 2017, 154 (04)
  • [3] WISE Y DWARFS AS PROBES OF THE BROWN DWARF- EXOPLANET CONNECTION
    Beichman, C.
    Gelino, Christopher R.
    Kirkpatrick, J. Davy
    Cushing, Michael C.
    Dodson-Robinson, Sally
    Marley, Mark S.
    Morley, Caroline V.
    Wright, E. L.
    [J]. ASTROPHYSICAL JOURNAL, 2014, 783 (02)
  • [4] THE SOLAR NEIGHBORHOOD. XXXVII. THE MASS-LUMINOSITY RELATION FOR MAIN-SEQUENCE M DWARFS
    Benedict, G. F.
    Henry, T. J.
    Franz, O. G.
    McArthur, B. E.
    Wasserman, L. H.
    Jao, Wei-Chun
    Cargile, P. A.
    Dieterich, S. B.
    Bradley, A. J.
    Nelan, E. P.
    Whipple, A. L.
    [J]. ASTRONOMICAL JOURNAL, 2016, 152 (05)
  • [5] Interferometric astrometry of Proxima Centauri and Barnard's star using Hubble Space Telescope Fine Guidance Sensor 3:: Detection limits for substellar companions
    Benedict, GF
    McArthur, B
    Chappell, DW
    Nelan, E
    Jefferys, WH
    van Altena, W
    Lee, J
    Cornell, D
    Shelus, PJ
    Hemenway, PD
    Franz, OG
    Wasserman, LH
    Duncombe, RL
    Story, D
    Whipple, AL
    Fredrick, LW
    [J]. ASTRONOMICAL JOURNAL, 1999, 118 (02) : 1086 - 1100
  • [6] Photometry of Proxima Centauri and Barnard's star using Hubble Space Telescope fine guidance sensor 3: A search for periodic variations
    Benedict, GF
    McArthur, B
    Nelan, E
    Story, D
    Whipple, AL
    Shelus, PJ
    Jefferys, WH
    Hemenway, PD
    Franz, OG
    Wasserman, LH
    Duncombe, RL
    van Altena, W
    Fredrick, LW
    [J]. ASTRONOMICAL JOURNAL, 1998, 116 (01) : 429 - 439
  • [7] BESSEL MS, 1990, ASTRON ASTROPHYS SUP, V83, P357
  • [8] Discovery of a brown dwarf very close to the Sun: A methane-rich brown dwarf companion to the low-mass star SCR 1845-6357
    Biller, BA
    Kasper, M
    Close, LM
    Brandner, W
    Kellner, S
    [J]. ASTROPHYSICAL JOURNAL, 2006, 641 (02) : L141 - L144
  • [9] Possible astrometric discovery of a substellar companion to the closest binary brown dwarf system WISE J104915.57-531906.1
    Boffin, H. M. J.
    Pourbaix, D.
    Muzic, K.
    Ivanov, V. D.
    Kurtev, R.
    Beletsky, Y.
    Mehner, A.
    Berger, J. P.
    Girard, J. H.
    Mawet, D.
    [J]. ASTRONOMY & ASTROPHYSICS, 2014, 561
  • [10] The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample
    Bonfils, X.
    Delfosse, X.
    Udry, S.
    Forveille, T.
    Mayor, M.
    Perrier, C.
    Bouchy, F.
    Gillon, M.
    Lovis, C.
    Pepe, F.
    Queloz, D.
    Santos, N. C.
    Segransan, D.
    Bertaux, J. -L
    [J]. ASTRONOMY & ASTROPHYSICS, 2013, 549