Pi Pavonis: Difference between revisions
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{{Short description|Astrometric binary star system in the constellation Pavo}} |
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{{Starbox character |
{{Starbox character |
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| type = |
| type = |
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| class = kA4hF0mF2 III<ref name=Gray1989/> |
| class = kA4hF0mF2 III<ref name=Gray1989/> |
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| b-v = +0.23<ref name=MermiliodUBV/> |
| b-v = +0.23<ref name=MermiliodUBV/> |
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| u-b = +0.17<ref name=MermiliodUBV/> |
| u-b = +0.17<ref name=MermiliodUBV/> |
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}} |
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{{Starbox catalog |
{{Starbox catalog |
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| names = {{odlist | B=π Pav | −63°4292 | FK5=3437 | HD=165040 | HIP=88866 | HR=6745 | SAO=254147 | GC=24665 }}<ref name=SIMBAD/> |
| names = {{odlist | B=π Pav | CPD=−63°4292 | FK5=3437 | HD=165040 | HIP=88866 | HR=6745 | SAO=254147 | GC=24665 }}<ref name=SIMBAD/> |
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}} |
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{{Starbox reference |
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'''π |
'''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 [[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 km/s.<ref name=Wilson1953/> |
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The visible component is an [[ |
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 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/> 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 K.<ref name=GaiaDR2/> |
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==References== |
==References== |
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{{reflist|refs= |
{{reflist|refs= |
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<ref name=SIMBAD>{{cite simbad | title=pi Pav | |
<ref name=SIMBAD>{{cite simbad | title=pi Pav | access-date=2019-10-12 }}</ref> |
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<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 |
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| bibcode=2008MNRAS.389..869E | arxiv=0806.2878 |
| bibcode=2008MNRAS.389..869E | arxiv=0806.2878 |
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| 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> |
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<ref name=Erspamer2003>{{cite journal |
<ref name=Erspamer2003>{{cite journal |
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| journal=Astronomy and Astrophysics |
| journal=Astronomy and Astrophysics |
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| volume=398 | pages=1121–1135 | date=February 2003 |
| volume=398 | pages=1121–1135 | date=February 2003 |
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| arxiv=astro-ph/0210065 | bibcode=2003A&A...398.1121E |
| issue=3 | arxiv=astro-ph/0210065 | bibcode=2003A&A...398.1121E |
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| doi=10.1051/0004-6361:20021711 }}</ref> |
| doi=10.1051/0004-6361:20021711 | s2cid=1109164 }}</ref> |
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<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 |
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| volume=10 | pages=183–196 | date=June 1989 |
| volume=10 | pages=183–196 | date=June 1989 |
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| doi=10.1007/BF02719315 | bibcode=1989JApA...10..183L }}</ref> |
| issue=2 | doi=10.1007/BF02719315 | bibcode=1989JApA...10..183L | s2cid=121258394 }}</ref> |
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<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= |
<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> |
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<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> |
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<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| |
<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> |
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<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| |
<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> |
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<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. |
<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> |
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<ref name=Wilson1953>{{cite |
<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> |
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<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> |
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<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. |
<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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}} |
}} |
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{{Stars of Pavo}} |
{{Stars of Pavo}} |
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{{DEFAULTSORT:Pi Pavonis}} |
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[[Category:A-type giants]] |
[[Category:A-type giants]] |
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[[Category: |
[[Category:Am stars]] |
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[[Category:Pavo (constellation)]] |
[[Category:Pavo (constellation)]] |
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[[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]] |
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[[Category:Hipparcos objects|088866]] |
[[Category:Hipparcos objects|088866]] |
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[[Category: |
[[Category:Bright Star Catalogue objects|6745]] |
Latest revision as of 01:29, 23 August 2024
Observation data Epoch J2000 Equinox J2000 | |
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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] |
Distance | 130.0 ± 0.9 ly (39.9 ± 0.3 pc) |
Absolute magnitude (MV) | 1.33[2] |
Details | |
Mass | 2.15[6] M☉ |
Radius | 2.84+0.42 −0.03[7] R☉ |
Luminosity | 24.69±0.36[7] L☉ |
Surface gravity (log g) | 3.81[8] cgs |
Temperature | 7,632+50 −510[7] K |
Metallicity [Fe/H] | 0.27[8] dex |
Rotational velocity (v sin i) | 30.0[9] km/s |
Age | 630[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
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]- ^ 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
- ^ 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
- ^ 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.
- ^ 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
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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
- ^ "pi Pav". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-12.
- ^ 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.
- ^ 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.
- ^ 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.