가까운 항성 목록: 두 판 사이의 차이
내용 삭제됨 내용 추가됨
편집 요약 없음 |
잔글 로봇이 더함: uk:Найближчі зорі; 예쁘게 바꿈 |
||
71번째 줄:
| {{RA|14|39|36.5}}
| {{DEC|−60|50|02}}
| rowspan="2" align=left | 0.747 23(1 17)″<ref name="Y"/><ref name="S">[http://adsabs.harvard.edu/abs/1999A%26A...341..121S Visual binary orbits and masses post Hipparcos], Staffan Söderhjelm, ''Astronomy and Astrophysics'' '''341''' (1999-01), pp.
| rowspan="2" | 4.3650(68)
| rowspan="2" |
88번째 줄:
| 9.53<ref name=RECONS />
| 13.22<ref name=RECONS />
| align=left | 3,134(102)<ref>[http://adsabs.harvard.edu/abs/2004AJ....127.2909D Barnard's Star and the M Dwarf Temperature Scale], P. C. Dawson and M. M. de Robertis, ''The Astronomical Journal'' '''127''', #5 (May 2004), pp.
| {{RA|17|57|48.5}}
| {{DEC|+04|41|36}}
104번째 줄:
| 제목=Spectral energy distribution for GJ406
| 저널=Astronomy and Astrophysics
| 발행년도=2006 | 발행월=02 | volume=447 | issue=2 | 쪽=
| url=http://adsabs.harvard.edu/abs/2006A&A...447..709P
| doi=10.1051/0004-6361:20052979 }}</ref>
118번째 줄:
| 7.47<ref name=RECONS />
| 10.44<ref name=RECONS />
| align=left | 3,400<ref>[http://adsabs.harvard.edu/abs/2002A&A...396..967P Carbon monoxide bands in M dwarfs], Y. V. Pavlenko and H. R. A. Jones, ''Astronomy and Astrophysics'' '''396''' (December 2002), pp.
| {{RA|11|03|20.2}}
| {{DEC|+35|58|12}}
131번째 줄:
| −1.43<ref name=RECONS />
| 1.47<ref name=RECONS />
| align=left | 9,940(210)<ref>[http://adsabs.harvard.edu/abs/2004IAUS..224....1A The physical properties of normal A stars], Saul J. Adelman, pp.
| rowspan="2" | {{RA|06|45|08.9}}
| rowspan="2" | {{DEC|−16|42|58}}
142번째 줄:
| 8.44<ref name=RECONS />
| 11.34<ref name=RECONS />
| align=left | 25,000(200)<ref>[http://adsabs.harvard.edu/abs/2005ApJ...630L..69L The Age and Progenitor Mass of Sirius B], James Liebert, Patrick A. Young, David Arnett, J.B. Holberg, and Kurtis A. Williams, ''The Astrophysical Journal'' '''630''', #1 (2005년 9월), pp.
|-
| rowspan="2" style="background: lightblue;" | 6
389번째 줄:
| align=left | 0.272 01(1 30)″<ref name="recent">RECONS가 이 항성계의 시차를 삼각법을 이용하여 최초로 정확하게 쟀다.</ref>
| 11.991(57)
| <ref name=henry1997>[http://adsabs.harvard.edu/abs/1997AJ....114..388H The solar neighborhood IV: discovery of the twentieth nearest star], Todd J. Henry, Philip A. Ianna, J. Davy Kirkpatrick, Hartmut Jahreiss, ''The Astronomical Journal'' '''114''', #1 (July 1997), pp.
|-
| style="background: lightblue;" | 21
441번째 줄:
|-
| style="background: lightblue;" | SCR 1845-6357 B
| style="background: #FF4080;" | [[갈색 왜성|T6]]<ref name=nearmt>[http://adsabs.harvard.edu/abs/2007A%26A...471..655K The very nearby M/T dwarf binary SCR 1845-6357], Markus Kasper, Beth A. Biller, Adam Burrows, Wolfgang Brandner, Jano Budaj, and Laird M. Close, ''Astronomy and Astrophysics'' '''471''', #2 (August 2007), pp.
| ''?''
| ''?''
501번째 줄:
| align=left | 0.247 71(1 55)″<ref name="recent"/>
| 13.167(82)
| <ref>[http://adsabs.harvard.edu/abs/2005AJ....129.1954J The Solar Neighborhood. XIII. Parallax Results from the CTIOPI 0.9 Meter Program: Stars with μ >= 1.0" yr<sup>-1</sup> (Motion sample)], Wei-Chun Jao, Todd J. Henry, John P. Subasavage, Misty A. Brown, Philip A. Ianna, Jennifer L. Bartlett, Edgardo Costa, René A. Méndez, ''The Astronomical Journal'' '''129''', #4 (April 2005), pp.
|-
| rowspan="2" style="background: lightblue;" | 29
767번째 줄:
| {{RA|03|39|35.2}}
| {{DEC|−35|25|41}}
| align=left | 0.201 40(4 20)″<ref name="T">[http://cdsads.u-strasbg.fr/abs/1996MNRAS.281..644T CCD astrometry of southern very low-mass stars], C. G. Tinney, ''Monthly Notices of the Royal Astronomical Society'' '''281''', #2 (July 1996), pp.
| 16.195(338)
|
783번째 줄:
| <ref name=costa2005 />
|-
!colspan="11"|시차 오차 범위 = 0.
|-
| style="background: lightblue;" | 49
859번째 줄:
[[sr:Spisak najbližih zvezda]]
[[tr:Yakın yıldızlar dizini]]
[[uk:Найближчі зорі]]
[[zh:恆星距離列表]]
| |||