请输入您要查询的百科知识:

 

词条 HD 42818
释义

  1. References

{{Starbox begin
| name = HD 42818
}}{{Starbox observe
| epoch = J2000
| constell = Camelopardalis
| ra = {{RA|06|18|50.7809}}[1]
| dec = {{DEC|+69|19|11.176}}[1]
| appmag_v = +4.76[3]
}}{{Starbox character
| type =
| class = A0 Vn[4]
| b-v = {{Val|0.025|0.003}}
| variable =
}}{{Starbox astrometry
| radial_v = {{Val|−7.0|7.4}}[5]
| prop_mo_ra = +0.686[1]
| prop_mo_dec = −108.270[1]
| parallax = 18.64
| p_error = 0.23
| parallax_footnote = [8]
| absmag_v = +1.11[3]
}}{{Starbox detail
| source =
| component1 = HD 42818 A
| mass = 2.49[10]
| radius = 2.7[11]
| luminosity = 33.83[3]
| gravity = {{Val|4.18|0.14}}[10]
| temperature = {{Val|10834|368|fmt=commas}}[10]
| metal_fe = 0.3[15]
| rotational_velocity = 255[10]
| age_myr = 99[10]
}}{{Starbox catalog
| names = {{odlist | BD=+62° 628 | FK5=234 | HD=42818 | HIP=29997 | HR=2209 | SAO=13788 }}
}}{{Starbox reference
| Simbad = HD+42818
}}{{Starbox end}}

HD 42818 is a suspected astrometric binary[19] star system in the northern circumpolar constellation of Camelopardalis. It is visible to the naked eye with an apparent visual magnitude of +4.76.[3] Based upon an annual parallax shift of {{Val|18.64|0.23|ul=mas}} as seen from Earth's orbit,

[8] it is located some 175 light years away. The system appears to be moving closer with a heliocentric radial velocity of −7 km/s.[5] As of 2012, it is estimated that the system will make its closest approach to the Sun in 485,000 years at a distance of around {{Convert|51.87|pc|ly|order=flip|abbr=on}}.[3]

The visible member, designated component A, is an A-type main-sequence star with a stellar classification of A0 Vn,[4] where the 'n' indicates "nebulous" absorption lines due to rotation. It is spinning rapidly with a projected rotational velocity of 255 km/s[10] (van Belle (2012) lists 325 km/s), giving the star a pronounced equatorial bulge.[26] Although spectral type A stars are not expected to emit X-rays, the coordinates of this star is a source of X-ray emission with a luminosity of {{Val|120.4|e=20|u=W}}. This may be coming from a cooler, unseen companion.[27]

The primary has an estimated 2.49[10] times the mass of the Sun and about 2.7[11] times the Sun's radius. It is a relatively young star, about 99 million years old. The star is radiating 34 times the Sun's luminosity from its photosphere at an effective temperature of 10,834 K.[10]

References

1. ^{{citation | title=Validation of the new Hipparcos reduction | last1=van Leeuwen | first1=F. | postscript=. | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | year=2007 | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 }}
2. ^{{citation | 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 | postscript=. }}
3. ^{{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 Apparent Diameters and Absolute Radii of Stars (CADARS) | edition=Third | journal=Astronomy & Astrophysics | volume=367 | pages=521–24 | date=2001 | bibcode=2001A&A...367..521P | doi=10.1051/0004-6361:20000451 | arxiv=astro-ph/0012289 | postscript=. }}
4. ^{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E | postscript=. | arxiv=0806.2878 }}
5. ^{{citation | title=X-ray emission from A-type stars | last1=Schröder | first1=C. | last2=Schmitt | first2=J. H. M. M. | journal=Astronomy and Astrophysics | postscript=. | volume=475 | issue=2 | date=November 2007 | pages=677–684 | doi=10.1051/0004-6361:20077429 | bibcode=2007A&A...475..677S }}
6. ^{{citation | display-authors=1 | last1=Cowley | first1=A. | last2=Cowley | first2=C. | last3=Jaschek | first3=M. | last4=Jaschek | first4=C. | title=A study of the bright A stars. I. A catalogue of spectral classifications | journal=Astronomical Journal | postscript=. | volume=74 | pages=375–406 | date=April 1969 | doi=10.1086/110819 | bibcode=1969AJ.....74..375C }}
7. ^{{citation | 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 | postscript=. }}
8. ^{{citation | last1=van Belle | first1=Gerard T. | title=Interferometric observations of rapidly rotating stars | journal=The Astronomy and Astrophysics Review | volume=20 | issue=1 | page=51 | date=March 2012 | doi=10.1007/s00159-012-0051-2 | bibcode=2012A&ARv..20...51V | postscript=. | arxiv=1204.2572 }}
9. ^{{citation | title=A new method for the inversion of atmospheric parameters of A/Am stars | display-authors=1 | last1=Gebran | first1=M. | last2=Farah | first2=W. | last3=Paletou | first3=F. | last4=Monier | first4=R. | last5=Watson | first5=V. | journal=Astronomy & Astrophysics | volume=589 | pages=A83 | year=2016 | bibcode=2016A&A...589A..83G | postscript=. | doi=10.1051/0004-6361/201528052 | arxiv=1603.01146 }}
10. ^{{citation | title=Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties | last1=Brown | first1=A. G. A. | last2=Vallenari | first2=A. | last3=Prusti | first3=T. | last4=De Bruijne | first4=J. H. J. | last5=Mignard | first5=F. | last6=Drimmel | first6=R. | last7=Babusiaux | first7=C. | last8=Bailer-Jones | first8=C. A. L. | last9=Bastian | first9=U. | last10=Biermann | first10=M. | last11=Evans | first11=D. W. | last12=Eyer | first12=L. | last13=Jansen | first13=F. | last14=Jordi | first14=C. | last15=Katz | first15=D. | last16=Klioner | first16=S. A. | last17=Lammers | first17=U. | last18=Lindegren | first18=L. | last19=Luri | first19=X. | last20=o'Mullane | first20=W. | last21=Panem | first21=C. | last22=Pourbaix | first22=D. | last23=Randich | first23=S. | last24=Sartoretti | first24=P. | last25=Siddiqui | first25=H. I. | last26=Soubiran | first26=C. | last27=Valette | first27=V. | last28=Van Leeuwen | first28=F. | last29=Walton | first29=N. A. | last30=Aerts | first30=C. | display-authors=1 | journal=Astronomy and Astrophysics | volume=595 | at=A2 | year=2016 | arxiv=1609.04172 | bibcode=2016A&A...595A...2G | doi=10.1051/0004-6361/201629512 | postscript=. }}
11. ^{{citation | title=The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets | last1=David | first1=Trevor J. | last2=Hillenbrand | first2=Lynne A. | 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=. }}
[1][2][3][4][5][6][7][8][9][10][11]
}}{{Stars of Camelopardalis}}{{DEFAULTSORT:Hd 42818}}

7 : A-type main-sequence stars|Astrometric binaries|Camelopardalis (constellation)|Durchmusterung objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects

随便看

 

开放百科全书收录14589846条英语、德语、日语等多语种百科知识,基本涵盖了大多数领域的百科知识,是一部内容自由、开放的电子版国际百科全书。

 

Copyright © 2023 OENC.NET All Rights Reserved
京ICP备2021023879号 更新时间:2024/11/10 22:55:57