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{{Short description|Astrometric binary star system in the constellation Pavo}}
{{Starbox begin}}
{{Starbox begin}}
{{Starbox image
{{Starbox image
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{{Starbox character
{{Starbox character
| type =
| type =
| class = kA4hF0mF2 III<ref name=Gray1989/> {{nowrap|(A3-F1 Sr<ref name=Renson2009/>)}}
| class = kA4hF0mF2 III<ref name=Gray1989/>
| b-v = +0.23<ref name=MermiliodUBV/>
| b-v = +0.23<ref name=MermiliodUBV/>
| u-b = +0.17<ref name=MermiliodUBV/>
| u-b = +0.17<ref name=MermiliodUBV/>
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}}
}}
{{Starbox catalog
{{Starbox catalog
| names = {{odlist | B=π&nbsp;Pav | −63°4292 | FK5=3437 | HD=165040 | HIP=88866 | HR=6745 | SAO=254147 | GC=24665 }}<ref name=SIMBAD/>
| names = {{odlist | B=π&nbsp;Pav | CPD=−63°4292 | FK5=3437 | HD=165040 | HIP=88866 | HR=6745 | SAO=254147 | GC=24665 }}<ref name=SIMBAD/>
}}
}}
{{Starbox reference
{{Starbox reference
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{{Starbox end}}
{{Starbox end}}


'''π Pav''', Latinized as '''Pi Pavonis''', is a candidate [[astrometric binary]]<ref name=Eggleton2008/> [[star]] system in the [[constellation]] [[Pavo (constellation)|Pavo]]. It is a white-hued star that is visible to the naked eye as a faint point of light with an [[apparent visual magnitude]] of 4.33.<ref name=XHIP/> The distance to this object is 130&nbsp;[[light year]]s based on [[stellar parallax|parallax]],<ref name=vanLeeuwen2007/> but it is drifting closer to the Sun with a [[radial velocity]] of −15.6&nbsp;km/s.<ref name=Wilson1953/>
'''π Pavonis''', [[Latinisation of names|Latinized]] as '''Pi Pavonis''', is a candidate [[astrometric binary]]<ref name=Eggleton2008/> [[star]] system in the [[constellation]] [[Pavo (constellation)|Pavo]]. It is a white-hued star that is visible to the naked eye as a faint point of light with an [[apparent visual magnitude]] of 4.33.<ref name=XHIP/> The distance to this object is 130&nbsp;[[light year]]s based on [[stellar parallax|parallax]],<ref name=vanLeeuwen2007/> but it is drifting closer to the Sun with a [[radial velocity]] of −15.6&nbsp;km/s.<ref name=Wilson1953/>


The visible component is an [[Ap star]] that displays an abundance anomaly of strontium.<ref name=Loden1989/> Grey et al. (1989) classify it as kA4hF0mF2&nbsp;III,<ref name=Gray1989/> matching a [[giant star]] with the [[calcium K line]] of an A4 star, the [[hydrogen lines]] of a cooler F0 star, and the [[metallicity|metal lines]] of a F2 star. However, Loden and Sundman (1989) don't consider it to be a giant.<ref name=Loden1989/> It is 630<ref name=DeRosa2014/>&nbsp;million years old with 2.15<ref name=DeRosa2014/> times the [[mass of the Sun]] and 2.8<ref name=GaiaDR2/> times the [[Sun's radius]]. The star is radiating 24.7<ref name=GaiaDR2/> times the [[Sun's luminosity]] from its [[photosphere]] at an [[effective temperature]] of 7,632&nbsp;K.<ref name=GaiaDR2/>
The visible component is an [[chemically peculiar star]] that displays an abundance anomaly of strontium.<ref name=Loden1989/><ref name=Renson2009/> Grey et al. (1989) classify it as kA4hF0mF2&nbsp;III,<ref name=Gray1989/> matching a [[giant star|giant]] [[Am star]] with the [[calcium K line]] of an A4 star, the [[hydrogen lines]] of a cooler F0 star, and the [[metallicity|metal lines]] of a F2 star. However, Loden and Sundman (1989) don't consider it to be a giant and list it as an [[Ap star]].<ref name=Loden1989/> It is 630<ref name=DeRosa2014/>&nbsp;million years old with 2.15<ref name=DeRosa2014/> times the [[mass of the Sun]] and 2.8<ref name=GaiaDR2/> times the [[Sun's radius]]. The star is radiating 24.7<ref name=GaiaDR2/> times the [[Sun's luminosity]] from its [[photosphere]] at an [[effective temperature]] of 7,632&nbsp;K.<ref name=GaiaDR2/>


==References==
==References==
{{reflist|refs=
{{reflist|refs=


<ref name=SIMBAD>{{cite simbad | title=pi Pav | accessdate=2019-10-12 }}</ref>
<ref name=SIMBAD>{{cite simbad | title=pi Pav | access-date=2019-10-12 }}</ref>


<ref name=GaiaDR2>{{cite DR2|6630558558672843392}}</ref>
<ref name=GaiaDR2>{{cite DR2|6630558558672843392}}</ref>
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| volume=389 | issue=2 | pages=869–879 | date=September 2008
| volume=389 | issue=2 | pages=869–879 | date=September 2008
| bibcode=2008MNRAS.389..869E | arxiv=0806.2878
| bibcode=2008MNRAS.389..869E | arxiv=0806.2878
| doi=10.1111/j.1365-2966.2008.13596.x }}</ref>
| doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | s2cid=14878976 }}</ref>


<ref name=Erspamer2003>{{cite journal
<ref name=Erspamer2003>{{cite journal
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| journal=Astronomy and Astrophysics
| journal=Astronomy and Astrophysics
| volume=398 | pages=1121–1135 | date=February 2003
| volume=398 | pages=1121–1135 | date=February 2003
| arxiv=astro-ph/0210065 | bibcode=2003A&A...398.1121E
| issue=3 | arxiv=astro-ph/0210065 | bibcode=2003A&A...398.1121E
| doi=10.1051/0004-6361:20021711 }}</ref>
| doi=10.1051/0004-6361:20021711 | s2cid=1109164 }}</ref>


<ref name=Loden1989>{{cite journal
<ref name=Loden1989>{{cite journal
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| journal=Journal of Astrophysics and Astronomy
| journal=Journal of Astrophysics and Astronomy
| volume=10 | pages=183–196 | date=June 1989
| volume=10 | pages=183–196 | date=June 1989
| doi=10.1007/BF02719315 | bibcode=1989JApA...10..183L }}</ref>
| issue=2 | doi=10.1007/BF02719315 | bibcode=1989JApA...10..183L | s2cid=121258394 }}</ref>


<ref name=vanLeeuwen2007>{{cite journal | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653 | year=2007 | last1=Van Leeuwen | first1=F. }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%2088866 Vizier catalog entry]</ref>
<ref name=vanLeeuwen2007>{{cite journal | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | year=2007 | last1=Van Leeuwen | first1=F. | s2cid=18759600 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-S?HIP%2088866 Vizier catalog entry]</ref>


<ref name=XHIP>{{cite journal | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | title=XHIP: An extended hipparcos compilation | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | last1=Anderson | first1=E. | last2=Francis | first2=Ch. }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=V/137D/XHIP&HIP=88866 Vizier catalog entry]</ref>
<ref name=XHIP>{{cite journal | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | title=XHIP: An extended hipparcos compilation | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | s2cid=119257644 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=V/137D/XHIP&HIP=88866 Vizier catalog entry]</ref>


<ref name=Renson2009>{{cite journal|bibcode=2009A&A...498..961R|title=Catalogue of Ap, Hg ''Mn'' and Am stars|journal=Astronomy and Astrophysics|volume=498|issue=3|pages=961|author1=Renson|first1=P.|last2=Manfroid|first2=J.|year=2009|doi=10.1051/0004-6361/200810788|url=https://zenodo.org/record/890529/files/article.pdf}}</ref>
<ref name=Renson2009>{{cite journal|bibcode=2009A&A...498..961R|title=Catalogue of Ap, Hg ''Mn'' and Am stars|journal=Astronomy and Astrophysics|volume=498|issue=3|pages=961|last1=Renson|first1=P.|last2=Manfroid|first2=J.|year=2009|doi=10.1051/0004-6361/200810788|url=https://zenodo.org/record/890529|doi-access=free}}</ref>


<ref name=Gray1989>{{cite journal|bibcode=1989ApJS...69..301G|title=The early F-type stars - Refined classification, confrontation with Stromgren photometry, and the effects of rotation|journal=Astrophysical Journal Supplement Series|volume=69|pages=301|author1=Gray|first1=R. O.|last2=Garrison|first2=R. F.|year=1989|doi=10.1086/191315}}</ref>
<ref name=Gray1989>{{cite journal|bibcode=1989ApJS...69..301G|title=The early F-type stars - Refined classification, confrontation with Stromgren photometry, and the effects of rotation|journal=Astrophysical Journal Supplement Series|volume=69|pages=301|last1=Gray|first1=R. O.|last2=Garrison|first2=R. F.|year=1989|doi=10.1086/191315}}</ref>


<ref name=MermiliodUBV>{{cite journal | bibcode=2006yCat.2168....0M | title=VizieR Online Data Catalog: Homogeneous Means in the UBV System (Mermilliod 1991) | journal=VizieR On-line Data Catalog: II/168. Originally published in: Institut d'Astronomie | volume=2168 | author1=Mermilliod | first1=J. C. | year=2006 }}[http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=II/168/ubvmeans&LID=%2B100165040 Vizier catalog entry]</ref>
<ref name=MermiliodUBV>{{cite journal | bibcode=2006yCat.2168....0M | title=VizieR Online Data Catalog: Homogeneous Means in the UBV System (Mermilliod 1991) | journal=VizieR On-line Data Catalog: II/168. Originally Published in: Institut d'Astronomie | volume=2168 | last1=Mermilliod | first1=J. C. | year=2006 }}[http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=II/168/ubvmeans&LID=%2B100165040 Vizier catalog entry]</ref>


<ref name=Wilson1953>{{cite book | last=Wilson | first=R. E. | year=1953 | title=General Catalogue of Stellar Radial Velocities | publisher=[[Carnegie Institution of Washington]] | bibcode=1953GCRV..C......0W | lccn=54001336 }}</ref>
<ref name=Wilson1953>{{cite journal | last=Wilson | first=R. E. | year=1953 | title=General Catalogue of Stellar Radial Velocities | journal=Carnegie Institute Washington D.C. Publication | publisher=[[Carnegie Institution of Washington]] | bibcode=1953GCRV..C......0W | lccn=54001336 }}</ref>


<ref name=DeRosa2014>{{cite journal | bibcode=2014MNRAS.437.1216D | doi=10.1093/mnras/stt1932 | arxiv=1311.7141| title=The VAST Survey - III. The multiplicity of A-type stars within 75 pc | journal=Monthly Notices of the Royal Astronomical Society | volume=437 | issue=2 | pages=1216 | year=2013 | last1=De Rosa | first1=R. J. | last2=Patience | first2=J. | last3=Wilson | first3=P. A. | last4=Schneider | first4=A. | last5=Wiktorowicz | first5=S. J. | last6=Vigan | first6=A. | last7=Marois | first7=C. | last8=Song | first8=I. | last9=MacIntosh | first9=B. | last10=Graham | first10=J. R. | last11=Doyon | first11=R. | last12=Bessell | first12=M. S. | last13=Thomas | first13=S. | last14=Lai | first14=O. }}</ref>
<ref name=DeRosa2014>{{cite journal | bibcode=2014MNRAS.437.1216D | doi=10.1093/mnras/stt1932 | arxiv=1311.7141| title=The VAST Survey - III. The multiplicity of A-type stars within 75 pc | journal=Monthly Notices of the Royal Astronomical Society | volume=437 | issue=2 | pages=1216 | year=2013 | last1=De Rosa | first1=R. J. | last2=Patience | first2=J. | last3=Wilson | first3=P. A. | last4=Schneider | first4=A. | last5=Wiktorowicz | first5=S. J. | last6=Vigan | first6=A. | last7=Marois | first7=C. | last8=Song | first8=I. | last9=MacIntosh | first9=B. | last10=Graham | first10=J. R. | last11=Doyon | first11=R. | last12=Bessell | first12=M. S. | last13=Thomas | first13=S. | last14=Lai | first14=O. | doi-access=free }}</ref>


<ref name=Glebocki2005>{{cite journal | bibcode=2005yCat.3244....0G | title=VizieR Online Data Catalog: Catalog of Stellar Rotational Velocities (Glebocki+ 2005) | journal=VizieR On-line Data Catalog: III/244. Originally published in: 2005csss...13..571G; 2005yCat.3244....0G | volume=3244 | author1=Glebocki | first1=R. | last2=Gnacinski | first2=P. | year=2005 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=III/244/catalog&HIP=88866 Vizier catalog entry]</ref>
<ref name=Glebocki2005>{{cite journal | bibcode=2005yCat.3244....0G | title=VizieR Online Data Catalog: Catalog of Stellar Rotational Velocities (Glebocki+ 2005) | journal=VizieR On-line Data Catalog: III/244. Originally Published in: 2005csss...13..571G; 2005yCat.3244....0G | volume=3244 | last1=Glebocki | first1=R. | last2=Gnacinski | first2=P. | year=2005 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=III/244/catalog&HIP=88866 Vizier catalog entry]</ref>


}}
}}
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{{Stars of Pavo}}
{{Stars of Pavo}}


{{DEFAULTSORT:Pi Pavonis}}
[[Category:A-type giants]]
[[Category:A-type giants]]
[[Category:Ap star]]
[[Category:Am stars]]
[[Category:Pavo (constellation)]]
[[Category:Pavo (constellation)]]
[[Category:Bayer objects|Pavonis, Pi]]
[[Category:Bayer objects|Pavonis, Pi]]
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[[Category:Henry Draper Catalogue objects|165040]]
[[Category:Henry Draper Catalogue objects|165040]]
[[Category:Hipparcos objects|088866]]
[[Category:Hipparcos objects|088866]]
[[Category:HR objects|6745]]
[[Category:Bright Star Catalogue objects|6745]]

Latest revision as of 01:29, 23 August 2024

Pi Pavonis
Location of π Pavonis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Pavo
Right ascension 18h 08m 34.81459s[1]
Declination −63° 40′ 06.7906″[1]
Apparent magnitude (V) 4.33[2]
Characteristics
Spectral type kA4hF0mF2 III[3]
U−B color index +0.17[4]
B−V color index +0.23[4]
Astrometry
Radial velocity (Rv)−15.60[5] km/s
Proper motion (μ) RA: +18.02[1] mas/yr
Dec.: -207.57[1] mas/yr
Parallax (π)25.09 ± 0.17 mas[1]
Distance130.0 ± 0.9 ly
(39.9 ± 0.3 pc)
Absolute magnitude (MV)1.33[2]
Details
Mass2.15[6] M
Radius2.84+0.42
−0.03
[7] R
Luminosity24.69±0.36[7] L
Surface gravity (log g)3.81[8] cgs
Temperature7,632+50
−510
[7] K
Metallicity [Fe/H]0.27[8] dex
Rotational velocity (v sin i)30.0[9] km/s
Age630[6] Myr
Other designations
π Pav, CPD−63°4292, FK5 3437, GC 24665, HD 165040, HIP 88866, HR 6745, SAO 254147[10]
Database references
SIMBADdata

π Pavonis, Latinized as Pi Pavonis, is a candidate astrometric binary[11] star system in the constellation Pavo. It is a white-hued star that is visible to the naked eye as a faint point of light with an apparent visual magnitude of 4.33.[2] The distance to this object is 130 light years based on parallax,[1] but it is drifting closer to the Sun with a radial velocity of −15.6 km/s.[5]

The visible component is an chemically peculiar star that displays an abundance anomaly of strontium.[12][13] Grey et al. (1989) classify it as kA4hF0mF2 III,[3] matching a giant Am star with the calcium K line of an A4 star, the hydrogen lines of a cooler F0 star, and the metal lines of a F2 star. However, Loden and Sundman (1989) don't consider it to be a giant and list it as an Ap star.[12] It is 630[6] million years old with 2.15[6] times the mass of the Sun and 2.8[7] times the Sun's radius. The star is radiating 24.7[7] times the Sun's luminosity from its photosphere at an effective temperature of 7,632 K.[7]

References

[edit]
  1. ^ a b c d e f Van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600. Vizier catalog entry
  2. ^ a b c Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. S2CID 119257644. Vizier catalog entry
  3. ^ a b Gray, R. O.; Garrison, R. F. (1989). "The early F-type stars - Refined classification, confrontation with Stromgren photometry, and the effects of rotation". Astrophysical Journal Supplement Series. 69: 301. Bibcode:1989ApJS...69..301G. doi:10.1086/191315.
  4. ^ a b Mermilliod, J. C. (2006). "VizieR Online Data Catalog: Homogeneous Means in the UBV System (Mermilliod 1991)". VizieR On-line Data Catalog: II/168. Originally Published in: Institut d'Astronomie. 2168. Bibcode:2006yCat.2168....0M.Vizier catalog entry
  5. ^ a b Wilson, R. E. (1953). "General Catalogue of Stellar Radial Velocities". Carnegie Institute Washington D.C. Publication. Carnegie Institution of Washington. Bibcode:1953GCRV..C......0W. LCCN 54001336.
  6. ^ a b c d De Rosa, R. J.; Patience, J.; Wilson, P. A.; Schneider, A.; Wiktorowicz, S. J.; Vigan, A.; Marois, C.; Song, I.; MacIntosh, B.; Graham, J. R.; Doyon, R.; Bessell, M. S.; Thomas, S.; Lai, O. (2013). "The VAST Survey - III. The multiplicity of A-type stars within 75 pc". Monthly Notices of the Royal Astronomical Society. 437 (2): 1216. arXiv:1311.7141. Bibcode:2014MNRAS.437.1216D. doi:10.1093/mnras/stt1932.
  7. ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
  8. ^ a b Erspamer, D.; North, P. (February 2003). "Automated spectroscopic abundances of A and F-type stars using echelle spectrographs. II. Abundances of 140 A-F stars from ELODIE". Astronomy and Astrophysics. 398 (3): 1121–1135. arXiv:astro-ph/0210065. Bibcode:2003A&A...398.1121E. doi:10.1051/0004-6361:20021711. S2CID 1109164.
  9. ^ Glebocki, R.; Gnacinski, P. (2005). "VizieR Online Data Catalog: Catalog of Stellar Rotational Velocities (Glebocki+ 2005)". VizieR On-line Data Catalog: III/244. Originally Published in: 2005csss...13..571G; 2005yCat.3244....0G. 3244. Bibcode:2005yCat.3244....0G. Vizier catalog entry
  10. ^ "pi Pav". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-12.
  11. ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008). "A catalogue of multiplicity among bright stellar systems". Monthly Notices of the Royal Astronomical Society. 389 (2): 869–879. arXiv:0806.2878. Bibcode:2008MNRAS.389..869E. doi:10.1111/j.1365-2966.2008.13596.x. S2CID 14878976.
  12. ^ a b Loden, L. O.; Sundman, A. (June 1989). "Giant CP stars?". Journal of Astrophysics and Astronomy. 10 (2): 183–196. Bibcode:1989JApA...10..183L. doi:10.1007/BF02719315. S2CID 121258394.
  13. ^ Renson, P.; Manfroid, J. (2009). "Catalogue of Ap, Hg Mn and Am stars". Astronomy and Astrophysics. 498 (3): 961. Bibcode:2009A&A...498..961R. doi:10.1051/0004-6361/200810788.