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词条 Psi7 Aurigae
释义

  1. References

  2. External links

{{DISPLAYTITLE:Psi7 Aurigae}}

For other star systems with this Bayer designation, see Psi Aurigae.

{{Starbox begin
| name = Psi7 Aurigae
}}{{Starbox image
| image={{Location mark
|image=Auriga constellation map.svg|alt=|float=center|width=260
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=ψ7 Aurigae
|x=112|y=354
}}
|caption=Location of ψ7 Aurigae (circled)
}}{{Starbox observe
| epoch = J2000
| ra = {{RA|06|50|45.94330}}
| dec = {{DEC|+41|46|52.4267}}
| appmag_v = 5.02[3]
| constell = Auriga
}}{{Starbox character
| class = K3 III[4]
| r-i = 0.46
| v-r =
| b-v = +1.27[3]
| u-b = +1.35[3]
| variable =
}}{{Starbox astrometry
| radial_v = {{nowrap|+59.53 ± 0.25}}[7]
| prop_mo_ra = –25.660[8]
| prop_mo_dec = –138.163[8]
| parallax = 9.8872
| p_error = 0.1499
| parallax_footnote = [8]
| absmag_v = −0.33[11]
}}{{Starbox detail
| mass =
| radius = 24[12]
| luminosity = 217[11]
| temperature = 4,300[14]
| metal_fe = 0.00[14]
| gravity = 2.35[14]
| rotational_velocity = 10[17]
| age_myr =
}}{{Starbox catalog
| names = ψ7 Aur, 58 Aurigae, BD+41 1536, FK5 2527, HD 49520, HIP 32844, HR 2516, SAO 41380.[18]
}}{{Starbox reference
|Simbad=58+Aur
}}{{Starbox end}}

Psi7 Aurigae, Latinized from ψ7 Aurigae, is a star in the northern constellation of Auriga. It is a dim, naked eye star with an apparent visual magnitude of 5.02. Based upon Gaia Data Release 2 parallax values, it is approximately {{Convert|330|ly|pc|abbr=off|lk=on}} from Earth.

ψ7 Aurigae is a giant star with a stellar classification of K3 III.[4] The measured angular diameter of this star, after correction for limb darkening, is {{nowrap|1.96 ± 0.04 mas}}.[20] At its estimated distance, this yields a physical size of about 24 times the radius of the Sun.[12] The outer envelope has an effective temperature of 4,300,[14] giving it an orange colour and a classification as a K-type star.[24] Although cooler than the sun, its larger size means that it is more luminous, emitting in total 217 times as much electromagnetic radiation.

References

1. ^{{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=. }}
2. ^{{citation | display-authors=1 | last1=Famaey | first1=B. | last2=Jorissen | first2=A. | last3=Luri | first3=X. | last4=Mayor | first4=M. | last5=Udry | first5=S. | last6=Dejonghe | first6=H. | last7=Turon | first7=C. | title=Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters | journal=Astronomy and Astrophysics | volume=430 | issue=1 | pages=165–186 |date=January 2005 | doi=10.1051/0004-6361:20041272 | bibcode=2005A&A...430..165F | arxiv=astro-ph/0409579 | postscript=. }}
3. ^{{citation | last=McWilliam | first=Andrew | title=High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances | journal=Astrophysical Journal Supplement Series | volume=74 | pages=1075–1128 |date=December 1990 | doi=10.1086/191527 | bibcode=1990ApJS...74.1075M | postscript=. }}
4. ^{{citation | title=The Spectra of the Bright Stars of Types F5-K5 | last=Roman | first=Nancy G. | journal=Astrophysical Journal | volume=116 | page=122 |date=July 1952 | doi=10.1086/145598 | bibcode=1952ApJ...116..122R | postscript=. }}
5. ^{{citation | last1=Bernacca | first1=P. L. | last2=Perinotto | first2=M. | title=A catalogue of stellar rotational velocities | journal=Contributi Osservatorio Astronomico di Padova in Asiago | volume=239 | issue=1 | date=1970 | bibcode=1970CoAsi.239....1B | postscript=. }}
6. ^{{citation | last1=Johnson | display-authors=1 | first1=H. L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | date=1966 | bibcode=1966CoLPL...4...99J }}
7. ^{{cite simbad | title=* 58 Aur | accessdate=2012-08-24 | postscript=. }}
8. ^{{citation | last1=Richichi | first1=A. | last2=Percheron | first2=I. | last3=Khristoforova | first3=M. | title=CHARM2: An updated Catalog of High Angular Resolution Measurements | journal=Astronomy and Astrophysics | volume=431 | pages=773–777 |date=February 2005 | doi=10.1051/0004-6361:20042039 | bibcode=2005A&A...431..773R }}
9. ^{{citation | first1=Kenneth R. | last1=Lang | title=Astrophysical formulae | volume=1 | series=Astronomy and astrophysics library | edition=3rd | publisher=Birkhäuser | date=2006 | isbn=3-540-29692-1 | url=https://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 }}. The radius (R*) is given by::
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. ^{{cite DR2|951619690275198720}}
Note: see VizieR catalogue I/311.
[1][2][3][4][5][6][7][8][9][10][11]
}}

External links

  • HR 2516
  • CCDM J06508+4147
  • Image Psi7 Aurigae
{{Stars of Auriga}}

8 : Auriga (constellation)|K-type giants|Bayer objects|Flamsteed objects|Henry Draper Catalogue objects|Hipparcos objects|HR objects|Durchmusterung objects

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