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词条 19 Canum Venaticorum
释义

  1. References

{{Starbox begin
| name = 19 Canum Venaticorum
}}{{Starbox observe
| epoch = J2000
| constell = Canes Venatici
| ra = {{RA|13|15|31.95263}}[1]
| dec = {{DEC|+40|51|18.7516}}[1]
| appmag_v = 5.77[3] {{nowrap|(5.87 + 9.48)}}[4]
}}{{Starbox character
| type = main sequence[5]
| class = A7 V[6]
| b-v = {{Val|0.198|0.004}}[3]
| u-b =
| variable =
}}{{Starbox astrometry
| radial_v = {{Val|−21.1|2.6}}[8]
| prop_mo_ra = −113.761[1]
| prop_mo_dec = +19.858[1]
| parallax = 13.7210
| p_error = 0.1581
| parallax_footnote = [1]
| absmag_v = 1.42[3]
}}{{Starbox orbit
| reference = [13]
| period = 219.2
| axis = 0.745
| inclination = 44.5
| node = 22.2
| periastron = 2201.7
| eccentricity = 0.686
| periarg = 273.3
}}{{Starbox detail
| source =
| component1 = 19 CVn A
| mass = {{Val|2.06|0.03}}[5]
| radius = 2.5[15]
| luminosity = {{Val|25.5|1.9|1.8}}[5]
| temperature = {{Val|8048|274|fmt=commas}}[17]
| gravity = {{Val|4.09|0.14}}[17]
| metal_fe =
| rotational_velocity = 110[5]
| age_myr = 366[17]
}}{{Starbox catalog
| names = {{odlist | F=19 CVn | BD=+41° 2374 | FK5=461 | HD=115271 | HIP=64692 | HR=5004 | SAO=44531 | WDS=J13155+4051 }}
}}{{Starbox reference
| Simbad = 19+CVn
}}{{Starbox end}}19 Canum Venaticorum is a binary star[13] system in the northern constellation of Canes Venatici, located approximately 238 light years from Sun based on its parallax. It is dimly visible to the naked eye as a white-hued star with an apparent visual magnitude of 5.77.[3] The pair orbit each other with a period of 219.2 years and an eccentricity of 0.686.[13] The system is moving closer to the Earth with a heliocentric radial velocity of −21 km/s.[8]

The magnitude +5.87 primary, component A, is a A-type main-sequence star with a stellar classification of A7 V.[4] It is 366[17] million years old with twice[5] the mass of the Sun and 2.5[15] times the Sun's radius. The star is radiating 25.5[5] times the Sun's luminosity from its photosphere at an effective temperature of 8,048 K.[17] It has a high rate of spin, showing a projected rotational velocity of 110 km/s.[5] As of 2012, its companion, designated component B, is a magnitude 9.48 star located {{Val|0.60|u=arcseconds}} from the primary along a position angle of 58°.[4]

References

1. ^{{cite DR2|1524888216726645248}}
2. ^{{citation | last1=Appenzeller | first1=Immo | postscript=. | title=MK Spectral Types for 185 Bright Stars | journal=Publications of the Astronomical Society of the Pacific | volume=79 | issue=467 | page=102 | date=April 1967 | doi=10.1086/128449 | bibcode=1967PASP...79..102A }}
3. ^{{cite journal | 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 }}
4. ^{{cite book | display-authors=1 | last1=Mason | first1=B. D. | last2=Wycoff | first2=G. L. I. | last3=Hartkopf | first3=W. I. | last4=Douglass | first4=G. G. | last5=Worley | first5=C. E. | title=The Washington Visual Double Star Catalog (WDS), Version 2019-01-21 | journal=The Astronomical Journal | volume=122 | issue=6 | pages=3466–3471 | date=December 2001 | doi=10.1086/323920 | bibcode=2001AJ....122.3466M | publisher=U. S. Naval Observatory, Washington D.C. }}
5. ^{{cite journal | last1=de Bruijne | first1=J. H. J. | last2=Eilers | first2=A.-C. | title=Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project | journal=Astronomy & Astrophysics | volume=546 | id=A61 | pages=14 | date=October 2012 | doi=10.1051/0004-6361/201219219 | bibcode=2012A&A...546A..61D | arxiv=1208.3048 }}
6. ^{{cite journal | title=Fundamental parameters of nearby stars from the comparison with evolutionary calculations: masses, radii and effective temperatures | last1=Allende Prieto | first1=C. | last2=Lambert | first2=D. L. | journal=Astronomy and Astrophysics | volume=352 | pages=555–562 | date=1999 | bibcode=1999A&A...352..555A | arxiv=astro-ph/9911002 }}
7. ^{{cite journal | 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 | arxiv=1501.03154 | doi=10.1088/0004-637X/804/2/146 }}
8. ^{{citation | title=Double Stars Information Circular | volume=187 | date=October 2015 | publisher=International Astronomical Union, Commission G1 | url=http://www.astro.gsu.edu/wds/bsl/cir187.pdf | accessdate=2019-01-26 }}
9. ^{{cite journal | title=Rotational velocities of A-type stars. IV. Evolution of rotational velocities | last1=Zorec | first1=J. | last2=Royer | first2=F. | last3=Asplund | first3=Martin | last4=Cassisi | first4=Santi | last5=Ramirez | first5=Ivan | last6=Melendez | first6=Jorge | last7=Bensby | first7=Thomas | last8=Feltzing | first8=Sofia | display-authors=1 | journal=Astronomy and Astrophysics | volume=537 | pages=A120 | year=2012 | bibcode=2012A&A...537A.120Z | arxiv=1201.2052 | doi=10.1051/0004-6361/201117691 }}
[1][2][3][4][5][6][7][8][9]
}}{{Stars of Canes Venatici}}

8 : A-type main-sequence stars|Binary stars|Canes Venatici|Durchmusterung objects|Flamsteed objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects

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