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词条 HR 6594
释义

  1. References

{{Starbox begin
| name = HR 6594
}}{{Starbox observe
| epoch = J2000
| constell = Hercules
| ra = {{RA|17|41|58.63355}}
| dec = {{DEC|+15|57|08.7606}}
| appmag_v = 5.55[3]
}}{{Starbox character
| type = Main sequence[4]
| class = F4 Vw[5]
| b-v = +0.38[3]
| u-b = −0.05[3]
| variable =
}}{{Starbox astrometry
| radial_v = −43.7[8]
| prop_mo_ra = −7.71
| prop_mo_dec = +104.64
| parallax = 28.69
| p_error = 0.63
| parallax_footnote =
| absmag_v = 2.74[12]
}}{{Starbox detail
| component1 = HR 6594 A
| mass = 1.34[13]
| radius = 0.97[14]
| luminosity_bolometric =
| gravity = 4.07[4]
| temperature = 6,615[4]
| metal_fe = −0.04[17]
| rotational_velocity = 31.7[4]
| rotation =
| age_gyr = 1.2[13]
}}{{Starbox catalog
| names = BD-16° 3256, HD 160910, HIP 86623, HR 6594, SAO 103033.[20]
}}{{Starbox reference
| Simbad = HR+6594
}}{{Starbox end}}HR 6594 is the Bright Star Catalogue designation for a binary star[21] system in the northern constellation of Hercules. It is faintly visible to the naked eye with an apparent visual magnitude of 5.55;[3] according to the Bortle scale, it is sufficiently bright to be visible from dark suburban skies. The distance to this system, as determined using parallax measurements, is about 114 light years. On the celestial sphere it is located near the star Alpha Ophiuchi; their projected separation is just 3 light years, although their actual separation is much greater.[24]

The primary is an F-type main sequence star with a stellar classification of F4 Vw, where the w indicates relatively weak metallic features in the ultraviolet spectrum.[5] This star has 134% of the Sun's mass,[13] but only 97% of the solar radius.[14] It is spinning with a projected rotational velocity of 31.7 km/s,[4] and is around 1.2 billion years old.[13] The effective temperature of the outer atmosphere is 6,615 K,[4] giving it the yellow-white hue of an F-type star.[31] The abundance of elements other than hydrogen or helium, what astronomers term the metallicity, is similar to that in the Sun.[17]

It has a magnitude 9.38 companion star orbiting with a 144-year period, a semimajor axis spanning 1.04 arcseconds, and an eccentricity of 0.42.[21] There is a third, visual companion of magnitude 14.46 at an angular separation of 154.70 arcseconds along a position angle of 271°, as of 2001.[34]

References

1. ^{{citation | last1=Mermilliod | first1=J.-C. | title=Compilation of Eggen's UBV data, transformed to UBV (unpublished) | publisher=SIMBAD | date=1986 | bibcode=1986EgUBV........0M | postscript=. }}
2. ^{{citation | display-authors=1 | last1=Schröder | first1=C. | last2=Reiners | first2=A. | last3=Schmitt | first3=J. H. M. M. | title=Ca II HK emission in rapidly rotating stars. Evidence for an onset of the solar-type dynamo | journal=Astronomy and Astrophysics | volume=493 | issue=3 | pages=1099–1107 | date=January 2009 | doi=10.1051/0004-6361:200810377 | bibcode=2009A&A...493.1099S | postscript=. | url=http://goedoc.uni-goettingen.de/goescholar/bitstream/handle/1/9690/aa10377-08.pdf?sequence=2}}
3. ^{{citation | title=Lithium in early F dwarfs | last1=Boesgaard | first1=A. M. | last2=Tripicco | first2=M. J. | journal=Astrophysical Journal, Part 1 | volume=303 | date=April 15, 1986 | pages=724–739 | doi=10.1086/164120 | bibcode=1986ApJ...303..724B | postscript=. }}
4. ^{{citation | display-authors=1 | 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 | volume=530 | issue=A138 | pages=21 | date=2011 | doi=10.1051/0004-6361/201016276 | bibcode=2011A&A...530A.138C | arxiv=1103.4651 | postscript=. }}
5. ^{{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 | postscript=. }}
6. ^{{citation | display-authors=1 | last1=Pasinetti-Fracassini | first1=L. E. | last2=Pastori | first2=L. | last3=Covino | first3=S. | last4=Pozzi | first4=A. | title=Catalogue of Stellar Diameters (CADARS) | journal=Astronomy and Astrophysics | volume=367 | pages=521–524 | date=February 2001 | doi=10.1051/0004-6361:20000451 | bibcode=2001A&A...367..521P | arxiv=astro-ph/0012289 | postscript=. }}
7. ^{{citation | title=Spectral Classification of A and F Stars | last1=Barry | first1=Don C. | journal=Astrophysical Journal Supplement | volume=19 | pages=281 | year=1970 | bibcode=1970ApJS...19..281B | doi=10.1086/190209 | postscript=. }}
8. ^{{citation | title=Dynamical masses of a selected sample of orbital binaries | last1=Malkov | first1=O. Yu. | last2=Tamazian | first2=V. S. | last3=Docobo | first3=J. A. | last4=Chulkov | first4=D. A. | journal=Astronomy & Astrophysics | display-authors=1 | volume=546 | id=A69 | pages=5 | date=October 2012 | doi=10.1051/0004-6361/201219774 | bibcode=2012A&A...546A..69M | postscript=. }}
9. ^{{citation | display-authors=1 | last1=Mason | first1=B. D. | last2=Wycoff | first2=G. L. | last3=Hartkopf | first3=W. I. | last4=Douglass | first4=G. G. | last5=Worley | first5=C. E. | title=The Washington Visual Double Star Catalog | year=2014 | bibcode=2001AJ....122.3466M | url=http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=B/wds | accessdate=2015-07-22 | doi = 10.1086/323920 | postscript=. | volume=122 | journal=The Astronomical Journal | pages=3466–3471}}
10. ^{{citation | title=The Colour of Stars | date=December 21, 2004 | work=Australia Telescope, Outreach and Education | publisher=Commonwealth Scientific and Industrial Research Organisation | url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html | accessdate=2012-01-16 | postscript=. }}
11. ^{{citation | title=Spitzer Limits on Dust Emission and Optical Gas Absorption Variability around Nearby Stars with Edge-on Circumstellar Disk Signatures | display-authors=1 | last1=Redfield | first1=Seth | last2=Kessler-Silacci | first2=Jacqueline E. | last3=Cieza | first3=Lucas A. | journal=The Astrophysical Journal | volume=661 | issue=2 | pages=944–971 | date=June 2007 | doi=10.1086/517516 | bibcode=2007ApJ...661..944R | arxiv=astro-ph/0703089 | postscript=. }}
12. ^{{citation | last=Wilson | first=R. E. | year=1953 | title=General Catalogue of Stellar Radial Velocities | publisher=Carnegie Institute of Washington D.C. | bibcode=1953GCRV..C......0W | postscript=. }}
13. ^{{cite simbad | title=HR 6594 | accessdate=2016-09-12 }}
[1][2][3][4][5][6][7][8][9][10][11][12][13]
}}{{Stars of Hercules|state=collapsed}}

7 : Hercules (constellation)|F-type main-sequence stars|Henry Draper Catalogue objects|Hipparcos objects|HR objects|Durchmusterung objects|Binary stars

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