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| epoch = J2000
| epoch = J2000
| constell = [[Octans]]
| constell = [[Octans]]
| ra = {{RA|10|59|13.757}}<ref name = GaiaDR2/>
| ra = {{RA|10|59|13.7578}}<ref name = EDR3/>
| dec = {{DEC|-84|35|38.02}}<ref name = GaiaDR2/>
| dec = {{DEC|-84|35|38.0177}}<ref name = EDR3/>
| appmag_v = 6.18{{±|0.01}}<ref name = Tycho2000/>
| appmag_v = 6.18{{±|0.01}}<ref name = Tycho2000/>
}}
}}
{{Starbox character
{{Starbox character
| class = A1 V<ref name = Houk1975/>
| type = [[main sequence]]<ref name = Zorec2012/>
| class = A1 Va<ref name = Paunzen2001/>
| u-b = +0.12<ref name = Johnson1966/>
| u-b = +0.12<ref name = Johnson1966/>
| b-v = +0.11<ref name = Johnson1966/>
| b-v = +0.11<ref name = Johnson1966/>
}}
}}
{{Starbox astrometry
{{Starbox astrometry
| radial_v = {{val|-47.69|0.02}}<ref name = Buder2019/>
| radial_v = −1.7{{±|0.6}}<ref name = Gontcharov2006/>
| prop_mo_ra = −65.708
| prop_mo_ra = −65.747
| prop_mo_dec = −8.177
| prop_mo_dec = −8.273
| pm_footnote = <ref name =GaiaDR2/>
| pm_footnote = <ref name = EDR3/>
| parallax = 9.1394
| parallax = 9.1133
| p_error = 0.0384
| p_error = 0.02
| parallax_footnote = <ref name = GaiaDR2/>
| parallax_footnote = <ref name = EDR3/>
| absmag_v = +1.08<ref name = XHIP/>
| absmag_v = +1.08<ref name = Anderson2012/>
}}
}}
{{Starbox detail
{{Starbox detail
| mass = {{val|2.37|0.03}}<ref name = Zorec2012/>
| mass = {{val|2.37|0.03}}<ref name = Zorec2012/>
| luminosity = {{val|45.3|3.1|3.0}}<ref name = Zorec2012/>
| luminosity = {{val|45.3|3.1|3.0}}<ref name = Zorec2012/>
| temperature = {{val|8974|167|164|fmt=commas}}<ref name = Zorec2012/>
| temperature = 9,500<ref name = Lafrasse2010/>
| rotational_velocity = 150<ref name = Zorec2012/>
| rotational_velocity = 152{{±|13}}<ref name = Reiners2004/>
| age_myr = {{val|376|22}}<ref name = Zorec2012/>
| age_myr = 547<ref name = Gontcharov2012/>
| radius = {{val|2.60|0.07|0.10}}<ref name = TIC/>
| radius = 2.6{{±|0.1}}<ref name = Stassun2019/>
| gravity = {{val|3.96|0.05|0.10}}<ref name = TIC/>
| gravity = 4.1<ref name = Lafrasse2010/>
| metal_fe = −0.21<ref name = Anders2019/>
| metal_fe = −0.01<ref name = Gontcharov2012/>
}}
}}
{{Starbox catalog
{{Starbox catalog
| names = {{odlist|B = η Octantis|HD = 96124|HIP = 53702|CPD = -83 386|HR = 4312|SAO = 258600}}
| names = {{odlist|B = η Oct|HD = 96124|HIP = 53702|CPD = −83°386|HR = 4312|SAO = 258600|FK5 = 1664|GC = 15164|Gould = 11 G. Octantis<ref name = Gould1879/>}}<ref name = SIMBAD/>
}}
}}
{{Starbox reference
{{Starbox reference
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{{Starbox end}}
{{Starbox end}}


'''Eta Octantis''', Latinized from '''η Octantis''', is a solitary star located in the southern [[circumpolar constellation]] [[Octans]]. With an [[apparent magnitude]] of about 6.19, it's barely visible to the [[naked eye]] under ideal conditions. The Star is located approximately {{convert|357|ly|pc}} away from the [[Solar System]], but is drifting closer with a heliocentric [[radial velocity]] of -47.69&nbsp;km/s.
'''Eta Octantis''', Latinized from '''η Octantis''', is a solitary [[star]] located in the southern [[circumpolar constellation]] [[Octans]]. It has an [[apparent magnitude]] of 6.19,<ref name = Tycho2000/> making it faintly visible to the [[naked eye]]. The object is situated at a distance of 358 [[light year]]s<ref name = EDR3/> but is approaching the [[Solar System]] with a heliocentric [[radial velocity]] of {{val|-1.7|ul=km/s}}.<ref name = Gontcharov2006/>


Eta Octantis is an [[A-type main sequence star]] with 2.37 times the [[Solar mass|Sun's mass]] and 2.6 times the [[Solar radius|Sun's radius]]. It radiates at 45.3 [[Solar luminosity|solar luminosities]] from its [[photosphere]] at an [[effective temperature]] of 8,974 [[Kelvin|K]]. Eta Octantis is a rapidly rotating star, with a [[projected rotational velocity]] of 150&nbsp;km/s, and is estimated to be 376 [[million years]] old, having completed about 70% of its life time.
Eta Octantis has a [[stellar classification]] of A1 Va,<ref name = Paunzen2001/> indicating that it is an ordinary [[A-type main sequence star]]. At present it has 2.37 times the [[Solar mass|Sun's mass]]<ref name = Zorec2012/> and 2.6 times the [[Solar radius|Sun's radius]].<ref name = Stassun2019/> It shines with a [[luminosity]] of {{val|45|ul=solar luminosity}}<ref name = Zorec2012/> from its [[photosphere]] at an [[effective temperature]] of 9,500 [[Kelvin|K]], giving a white hue.<ref name = Lafrasse2010/> Eta Octantis is a rapidly rotating star, with a [[projected rotational velocity]] of {{val|152|ul=km/s}},<ref name = Reiners2004/> and is estimated to be 547 [[million years]] old,<ref name = Gontcharov2012/> having completed 72% of its [[main sequence]] lifetime.<ref name = Zorec2012/>


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


<ref name = GaiaDR2>{{Cite DR2|5191251074311205888}}</ref>
<ref name = EDR3>{{Cite Gaia EDR3|5191251074311205888}}</ref>


<ref name = Johnson1966>{{cite journal |last1=Johnson |first1=H. L. |last2=Mitchell |first2=R. I. |last3=Iriarte |first3=B. |last4=Wisniewski |first4=W. Z. |title=UBVRIJKL Photometry of the Bright Stars |journal=Communications of the Lunar and Planetary Laboratory |date=1966 |volume=4 |pages=99–110 |bibcode=1966CoLPL...4...99J}}</ref>
<ref name = Johnson1966>{{cite journal |last1=Johnson |first1=H. L. |last2=Mitchell |first2=R. I. |last3=Iriarte |first3=B. |last4=Wisniewski |first4=W. Z. |title=UBVRIJKL Photometry of the Bright Stars |journal=Communications of the Lunar and Planetary Laboratory |date=1966 |volume=4 |pages=99–110 |bibcode=1966CoLPL...4...99J}}</ref>


<ref name = Tycho2000>{{cite journal |last1=Høg |first1=E. |last2=Fabricius |first2=C. |last3=Makarov |first3=V. V. |last4=Urban |first4=S. |last5=Corbin |first5=T. |last6=Wycoff |first6=G. |last7=Bastian |first7=U. |last8=Schwekendiek |first8=P. |last9=Wicenec |first9=A. |title=The Tycho-2 catalogue of the 2.5 million brightest stars |journal=Astronomy and Astrophysics |date=1 March 2000 |volume=355 |pages=L27–L30 |bibcode=2000A&A...355L..27H |issn=0004-6361}}</ref>
<ref name = Tycho2000>{{cite journal |last1=Høg |first1=E. |last2=Fabricius |first2=C. |last3=Makarov |first3=V. V. |last4=Urban |first4=S. |last5=Corbin |first5=T. |last6=Wycoff |first6=G. |last7=Bastian |first7=U. |last8=Schwekendiek |first8=P. |last9=Wicenec |first9=A. |title=The Tycho-2 catalogue of the 2.5 million brightest stars |journal=Astronomy and Astrophysics |date=March 2000 |volume=355 |pages=L27–L30 |issn=0004-6361 |bibcode=2000A&A...355L..27H}}</ref>


<ref name = Houk1975>{{cite journal |last1=Houk |first1=N. |last2=Cowley |first2=A. P. |title=University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations -90_ to -53_f0. |journal=University of Michigan Catalogue of Two-dimensional Spectral Types for the HD Stars. Volume I. Declinations -90_ to -53_f0., by Houk, N.; Cowley, A. P.. Ann Arbor, MI (USA): Department of Astronomy, University of Michigan, 19 + 452 P. |date=1975 |bibcode=1975mcts.book.....H }}</ref>
<ref name = Paunzen2001>{{cite journal | last1 = Paunzen | first1 = E. | last2 = Duffee | first2 = B. | last3 = Heiter | first3 = U. | last4 = Kuschnig | first4 = R. | last5 = Weiss | first5 = W. W. | title = A spectroscopic survey for <i>λ</i> Bootis stars | journal = Astronomy &amp; Astrophysics | date = July 2001 | volume = 373 | issue = 2 | pages = 625–632 | issn = 0004-6361 | eissn = 1432-0746 | doi = 10.1051/0004-6361:20010630 | bibcode = 2001A&A...373..625P | doi-access = free}}</ref>


<ref name = Gontcharov2006>{{cite journal |last1=Gontcharov |first1=G. A. |title=Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system |journal=Astronomy Letters |date=November 2006 |volume=32 |issue=11 |pages=759–771 |doi=10.1134/S1063773706110065 |issn=1063-7737 |bibcode=2006AstL...32..759G |arxiv=1606.08053|s2cid=119231169 }}</ref>
<ref name = Buder2019>{{cite journal |display-authors=1 |last1=Buder |first1=S. |last2=Lind |first2=K. |last3=Ness |first3=M. K. |last4=Asplund |first4=M. |last5=Duong |first5=L. |last6=Lin |first6=J. |last7=Kos |first7=J. |last8=Casagrande |first8=L. |last9=Casey |first9=A. R. |last10=Bland-Hawthorn |first10=J. |last11=de Silva |first11=G. M. |last12=D'Orazi |first12=V. |last13=Freeman |first13=K. C. |last14=Martell |first14=S. L. |last15=Schlesinger |first15=K. J. |last16=Sharma |first16=S. |last17=Simpson |first17=J. D. |last18=Zucker |first18=D. B. |last19=Zwitter |first19=T. |last20=Cotar |first20=K. |last21=Dotter |first21=A. |last22=Hayden |first22=M. R. |last23=Hyde |first23=E. A. |last24=Kafle |first24=P. R. |last25=Lewis |first25=G. F. |last26=Nataf |first26=D. M. |last27=Nordlander |first27=T. |last28=Reid |first28=W. |last29=Rix |first29=H.-W. |last30=Skúladóttir |first30=Á. |last31=Stello |first31=D. |last32=Ting |first32=Y.-S. |last33=Traven |first33=G. |last34=Wyse |first34=R. F. G. |title=The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS |journal=Astronomy and Astrophysics |date=1 April 2019 |volume=624 |pages=A19 |doi=10.1051/0004-6361/201833218 |arxiv=1804.05869 |bibcode=2019A&A...624A..19B |s2cid=102485610 |issn=0004-6361}}</ref>


<ref name = XHIP>{{cite journal |last1=Anderson |first1=E. |last2=Francis |first2=Ch. |title=XHIP: An extended hipparcos compilation |journal=Astronomy Letters |date=1 May 2012 |volume=38 |issue=5 |pages=331–346 |doi=10.1134/S1063773712050015 |arxiv=1108.4971 |bibcode=2012AstL...38..331A |s2cid=119257644 |issn=1063-7737}}</ref>
<ref name = Anderson2012>{{cite journal |last1=Anderson |first1=E. |last2=Francis |first2=Ch. |title=XHIP: An extended hipparcos compilation |journal=Astronomy Letters |date=May 2012 |volume=38 |issue=5 |pages=331–346 |doi=10.1134/S1063773712050015 |language=en |issn=1063-7737 |bibcode=2012AstL...38..331A |arxiv=1108.4971|s2cid=119257644 }}</ref>


<ref name = Zorec2012>{{cite journal |last1=Zorec |first1=J. |last2=Royer |first2=F. |title=Rotational velocities of A-type stars. IV. Evolution of rotational velocities |journal=Astronomy and Astrophysics |date=1 January 2012 |volume=537 |pages=A120 |doi=10.1051/0004-6361/201117691 |arxiv=1201.2052 |bibcode=2012A&A...537A.120Z |s2cid=55586789 |issn=0004-6361}}</ref>
<ref name = Zorec2012>{{cite journal |last1=Zorec |first1=J. |last2=Royer |first2=F. |title=Rotational velocities of A-type stars. IV. Evolution of rotational velocities |journal=Astronomy and Astrophysics |date=1 January 2012 |volume=537 |pages=A120 |doi=10.1051/0004-6361/201117691 |arxiv=1201.2052 |bibcode=2012A&A...537A.120Z |s2cid=55586789 |issn=0004-6361}}</ref>


<ref name = TIC>{{Cite journal|display-authors=1|last1=Stassun|first1=Keivan G.|last2=Oelkers|first2=Ryan J.|last3=Paegert|first3=Martin|last4=Torres|first4=Guillermo|last5=Pepper|first5=Joshua|last6=De Lee|first6=Nathan|last7=Collins|first7=Kevin|last8=Latham|first8=David W.|last9=Muirhead|first9=Philip S.|last10=Chittidi|first10=Jay|last11=Rojas-Ayala|first11=Bárbara|date=2019-10-01|title=The Revised TESS Input Catalog and Candidate Target List|bibcode=2019AJ....158..138S|journal=The Astronomical Journal|volume=158|issue=4|pages=138|doi=10.3847/1538-3881/ab3467|hdl=1721.1/124721|s2cid=166227927|issn=0004-6256|hdl-access=free}}</ref>
<ref name = Stassun2019>{{cite journal |display-authors=1 |last1=Stassun |first1=Keivan G. |last2=Oelkers |first2=Ryan J. |last3=Paegert |first3=Martin |last4=Torres |first4=Guillermo |last5=Pepper |first5=Joshua |last6=Lee |first6=Nathan De |last7=Collins |first7=Kevin |last8=Latham |first8=David W. |last9=Muirhead |first9=Philip S. |last10=Chittidi |first10=Jay |last11=Rojas-Ayala |first11=Bárbara |last12=Fleming |first12=Scott W. |last13=Rose |first13=Mark E. |last14=Tenenbaum |first14=Peter |last15=Ting |first15=Eric B. |last16=Kane |first16=Stephen R. |last17=Barclay |first17=Thomas |last18=Bean |first18=Jacob L. |last19=Brassuer |first19=C. E. |last20=Charbonneau |first20=David |last21=Ge |first21=Jian |last22=Lissauer |first22=Jack J. |last23=Mann |first23=Andrew W. |last24=McLean |first24=Brian |last25=Mullally |first25=Susan |last26=Narita |first26=Norio |last27=Plavchan |first27=Peter |last28=Ricker |first28=George R. |last29=Sasselov |first29=Dimitar |last30=Seager |first30=S. |last31=Sharma |first31=Sanjib |last32=Shiao |first32=Bernie |last33=Sozzetti |first33=Alessandro |last34=Stello |first34=Dennis |last35=Vanderspek |first35=Roland |last36=Wallace |first36=Geoff |last37=Winn |first37=Joshua N. |title=The Revised TESS Input Catalog and Candidate Target List |journal=The Astronomical Journal |date=9 September 2019 |volume=158 |issue=4 |pages=138 |doi=10.3847/1538-3881/ab3467 |issn=0004-6256 |bibcode=2019AJ....158..138S |arxiv=1905.10694 |doi-access=free}}</ref>


<ref name = Gontcharov2012>{{cite journal |last1=Gontcharov |first1=G. A. |title=Dependence of kinematics on the age of stars in the solar neighborhood |journal=Astronomy Letters |date=December 2012 |volume=38 |issue=12 |pages=771–782 |doi=10.1134/S1063773712120031 |issn=0320-0108 |bibcode=2012AstL...38..771G |arxiv=1606.08814}}</ref>
<ref name = Anders2019>{{Cite journal|display-authors=1|last1=Anders|first1=F.|last2=Khalatyan|first2=A.|last3=Chiappini|first3=C.|last4=Queiroz|first4=A. B.|last5=Santiago|first5=B. X.|last6=Jordi|first6=C.|last7=Girardi|first7=L.|last8=Brown|first8=A. G. A.|last9=Matijevic|first9=G.|last10=Monari|first10=G.|last11=Cantat-Gaudin|first11=T.|date=2019-08-01|title=Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18|bibcode=2019A&A...628A..94A|journal=Astronomy and Astrophysics|volume=628|pages=A94|doi=10.1051/0004-6361/201935765|arxiv=1904.11302|s2cid=131780028|issn=0004-6361}}</ref>

<ref name = Reiners2004>{{cite journal | last1 = Reiners | first1 = A. | last2 = Royer | first2 = F. | title = First signatures of strong differential rotation in A-type stars | journal = Astronomy &amp; Astrophysics | date = February 2004 | volume = 415 | issue = 1 | pages = 325–329 | issn = 0004-6361 | eissn = 1432-0746 | doi = 10.1051/0004-6361:20034175 | bibcode = 2004A&A...415..325R | arxiv = astro-ph/0311341 | doi-access = free}}</ref>

<ref name = Lafrasse2010>{{cite book |last1=Lafrasse |first1=Sylvain |last2=Mella |first2=Guillaume |last3=Bonneau |first3=Daniel |last4=Duvert |first4=Gilles |last5=Delfosse |first5=Xavier |last6=Chesneau |first6=Olivier |last7=Chelli |first7=Alain |title=Optical and Infrared Interferometry II |chapter=Building the 'JMMC Stellar Diameters Catalog' using SearchCal |date=16 July 2010 |volume=7734 |pages=77344E |doi=10.1117/12.857024 |bibcode=2010SPIE.7734E..4EL |arxiv=1009.0137|s2cid=32097037 }}</ref>

<ref name = Gould1879>{{cite journal | last=Gould | first=Benjamin Apthorp | title=Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas | journal=Resultados del Observatorio Nacional Argentino | volume=1 | bibcode=1879RNAO....1.....G | year=1878 | page=}}</ref>

<ref name = SIMBAD>{{Cite simbad|title = eta Oct|access-date = June 25, 2022}}</ref>


}}
}}

Revision as of 01:25, 26 June 2022

η Octantis
Location of η Octantis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Octans
Right ascension 10h 59m 13.7578s[1]
Declination −84° 35′ 38.0177″[1]
Apparent magnitude (V) 6.18±0.01[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A1 Va[4]
U−B color index +0.12[5]
B−V color index +0.11[5]
Astrometry
Radial velocity (Rv)−1.7±0.6[6] km/s
Proper motion (μ) RA: −65.747 mas/yr[1]
Dec.: −8.273 mas/yr[1]
Parallax (π)9.1133 ± 0.02 mas[1]
Distance357.9 ± 0.8 ly
(109.7 ± 0.2 pc)
Absolute magnitude (MV)+1.08[7]
Details
Mass2.37±0.03[3] M
Radius2.6±0.1[8] R
Luminosity45.3+3.1
−3.0
[3] L
Surface gravity (log g)4.1[9] cgs
Temperature9,500[9] K
Metallicity [Fe/H]−0.01[10] dex
Rotational velocity (v sin i)152±13[11] km/s
Age547[10] Myr
Other designations
η Oct, 11 G. Octantis[12], CPD−83°386, FK5 1664, GC 15164, HD 96124, HIP 53702, HR 4312, SAO 258600[13]
Database references
SIMBADdata

Eta Octantis, Latinized from η Octantis, is a solitary star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 6.19,[2] making it faintly visible to the naked eye. The object is situated at a distance of 358 light years[1] but is approaching the Solar System with a heliocentric radial velocity of −1.7 km/s.[6]

Eta Octantis has a stellar classification of A1 Va,[4] indicating that it is an ordinary A-type main sequence star. At present it has 2.37 times the Sun's mass[3] and 2.6 times the Sun's radius.[8] It shines with a luminosity of 45 L[3] from its photosphere at an effective temperature of 9,500 K, giving a white hue.[9] Eta Octantis is a rapidly rotating star, with a projected rotational velocity of 152 km/s,[11] and is estimated to be 547 million years old,[10] having completed 72% of its main sequence lifetime.[3]

References

  1. ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  2. ^ a b Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361.
  3. ^ a b c d e f Zorec, J.; Royer, F. (1 January 2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691. ISSN 0004-6361. S2CID 55586789.
  4. ^ a b Paunzen, E.; Duffee, B.; Heiter, U.; Kuschnig, R.; Weiss, W. W. (July 2001). "A spectroscopic survey for λ Bootis stars". Astronomy & Astrophysics. 373 (2): 625–632. Bibcode:2001A&A...373..625P. doi:10.1051/0004-6361:20010630. eISSN 1432-0746. ISSN 0004-6361.
  5. ^ a b Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
  6. ^ a b Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. ISSN 1063-7737. S2CID 119231169.
  7. ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. ISSN 1063-7737. S2CID 119257644.
  8. ^ a b Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. ISSN 0004-6256.
  9. ^ a b c Lafrasse, Sylvain; Mella, Guillaume; Bonneau, Daniel; Duvert, Gilles; Delfosse, Xavier; Chesneau, Olivier; Chelli, Alain (16 July 2010). "Building the 'JMMC Stellar Diameters Catalog' using SearchCal". Optical and Infrared Interferometry II. Vol. 7734. pp. 77344E. arXiv:1009.0137. Bibcode:2010SPIE.7734E..4EL. doi:10.1117/12.857024. S2CID 32097037.
  10. ^ a b c Gontcharov, G. A. (December 2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv:1606.08814. Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031. ISSN 0320-0108.
  11. ^ a b Reiners, A.; Royer, F. (February 2004). "First signatures of strong differential rotation in A-type stars". Astronomy & Astrophysics. 415 (1): 325–329. arXiv:astro-ph/0311341. Bibcode:2004A&A...415..325R. doi:10.1051/0004-6361:20034175. eISSN 1432-0746. ISSN 0004-6361.
  12. ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode:1879RNAO....1.....G.
  13. ^ "eta Oct". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved June 25, 2022.