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Epsilon Eridani: Revizyonlar arasındaki fark

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40. satır:
|tarih=Kasım 2007 | başlık=Validation of the new Hipparcos reduction | cilt=474 | sayı=2 | sayfalar=653–664 | bibcode=2007A&A...474..653V | arxiv=0708.1752v1 | doi=10.1051/0004-6361:20078357 | dergi=Astronomy and Astrophysics | postscript=. }} ''Note:'' see VizieR catalogue [http://vizier.u-strasbg.fr/viz-bin/Cat?I/311 I/311].</ref>
 
<ref name=SIMBADsaaoc8_59>{{kaynak | urlson1=http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V*+eps+EriCousins | başlıkilk1=V*A. epsW. EriJ. –| variablebaşlık=Standardization of BYBroadband DraPhotometry typeof |Equatorial iş=[[SIMBAD]]Standards | dergi=[[CentreSouth deAfrican DonnéesAstronomical astronomiquesObservatory deCirculars Strasbourg]]| cilt=8 | erişimtarihisayı=1559 Nisan| 2016yıl=1984 | bibcode=1984SAAOC...8...59C | postscript=. }}</ref>
 
<ref name=aj132_1_161>{{kaynak | display-authors=1 | son1=Gray | ilk1=R. O. | son2=Corbally | il2=C. J. | son3=Garrison | ilk3=R. F. | son4=McFadden | ilk4=M. T. | son5=Bubar | ilk5=E. J. | son6=McGahee | ilk6=C. E. | son7=O'Donoghue | ilk7=A. A. | son8=Knox | ilk8=E. R. | başlık=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample | dergi=[[The Astronomical Journal]] | cilt=132 | sayı=1 | sayfalar=161–170 |tarih=Temmuz 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | postscript=. }}</ref>
 
<ref name=SIMBAD>{{kaynak | url=http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=V*+eps+Eri | başlık=V* eps Eri – variable of BY Dra type | iş=[[SIMBAD]] | dergi=[[Centre de Données astronomiques de Strasbourg]] | erişimtarihi=15 Nisan 2016 | postscript=. }}</ref>
 
<ref name=gcvs>{{kaynak | başlık=GCVS query=eps Eri | yayımcı=[[Sternberg Astronomical Institute]], Moscow, Russia | iş=[[General Catalog of Variable Stars]] | url=http://www.sai.msu.su/groups/cluster/gcvs/cgi-bin/search.cgi?search=eps+Eri | erişimtarihi=15 Nisan 2016 | postscript=. }}</ref>
 
<ref name=rgcrv66>{{kaynak | som1=Evans | ilk1=D. S.| tarih=20–24 Haziran 1966 | yazarlar=Batten, Alan Henry; Heard, John Frederick | başlık=The revision of the general catalogue of radial velocities | iş=Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30 | sayfalar=[[Toronto Üniversitesi]] | yayımcı=[[International Astronomical Union]] | bibcode=1967IAUS...30...57E | cilt=30 | sayfalar=57 | postscript=. }}</ref>
 
<ref name=aj132_2206>{{kaynak | display-authors=1 | son1=Benedict | ilk1=G. Fritz | son2=McArthur | ilk2=Barbara E. | son3=Gatewood | ilk3=George | son4=Nelan | ilk4=Edmund | son5=Cochran | ilk5=William D. | son6=Hatzes | ilk6=Artie | son7=Endl | ilk7=Michael | son8=Wittenmyer | ilk8=Robert | son9=Baliunas | ilk9=Sallie L.| son10=Walker | ilk10=Gordon A. H. | son11=Yang | ilk11=Stephenson | son12=Kürster | ilk12=Martin | son13=Els | ilk13=Sebastian | son14=Paulson | ilk14=Diane B. |tarih=Kasım 2006 | başlık=The extrasolar planet e Eridani b – orbit and mass | dergi=The Astronomical Journal | cilt=132 | sayı=5 | sayfalar=2206–2218 | bibcode=2006AJ....132.2206B | doi=10.1086/508323 | arxiv=astro-ph/0610247 | postscript=. }}</ref>▼
 
<ref name=RECONS>{{kaynak | yazar=Staff | tarih=8 Haziran 2007 | url=http://www.astro.gsu.edu/RECONS/TOP100.posted.htm | başlık=The one hundred nearest star systems | publisher=[[Research Consortium On Nearby Stars]] | erişimtarihi=15 Nisan 2016 }}</ref>
 
<ref name=mnras403_3_1368"Janson2015">{{kaynak | display-authors=1| son1=GonzalezJanson | ilk1=G.Markus| son2=CarlsonQuanz | ilk2=M.Sascha KP. | son3=TobinCarson | ilk3=R.Joseph WC. | başlıkson4=ParentThalmann stars| ofilk4=Christian extrasolar| planetsson5=Lafrenière –| X.ilk5=David Lithium| abundancesson6=Amara and| vilk6=Adam sini revisited | dergibaşlık=[[MonthlyHigh-contrast imaging with Spitzer: deep Noticesobservations of theVega, RoyalFomalhaut, Astronomicaland ε Eridani | dergi=Astronomy & Society]]Astrophysics | cilt=403574 | sayıid=3A120 | sayfalar=1368–138010 | tarih=NisanŞubat 20102015 | doi=10.11111051/j.13650004-2966.2009.16195.x6361/201424944 | bibcode=2010MNRAS2015A&A...403574A.1368G120J | arxiv =0912 1412.16214816 | postscript=. }} See table 3.</ref>
 
<ref name=aaa505_1_205>{{kaynak | display-authors=1| son1=Demory | ilk1=B.-O.| son2=Ségransan | ilk2=D.| son3=Forveille | ilk3=T.| son4=Queloz | ilk4=D.| son5=Beuzit | ilk5=J.-L.| son6=Delfosse | ilk6=X.;| son7=di Folco | ilk7=E.| son8=Kervella | ilk8=P.| son9=Le Bouquin | ilk9=J.-B.| son10=Perrier | ilk10=C. | son11=Benisty | ilk11=M. | son12=Duvert | ilk12=G. | son13=Hofmann | ilk13=K.-H. | son14=Lopez | ilk14=B. | son15=Petrov | ilk15=R. | başlık=Mass-radius relation of low and very low-mass stars revisited with the VLTI | dergi=[[Astronomy and Astrophysics]] | cilt=505 | sayı=1 |tarih=Ekim 2009 | sayfalar=205–215 | doi=10.1051/0004-6361/200911976 | bibcode=2009A&A...505..205D | arxiv=0906.0602 | postscript=. }} See Table B.1</ref>
 
<ref name=apj460_993>{{kaynak | display-authors=1| son1=Saumon | ilk1=D.| son2=Hubbard | ilk2=W. B.| son3=Burrows | ilk3=A.| son4=Guillot6 | ilk4=T.| son5=Lunine | ilk5=J. I.| son6=Chabrier | ilk6=G.| url=http://articles.adsabs.harvard.edu/full/1996ApJ...460..993S| başlık=A theory of extrasolar giant planets | dergi=The Astrophysical Journal | cilt=460 | sayfa=993 |tarih=Nisan 1996 | doi=10.1086/177027 | bibcode=1996ApJ...460..993S | arxiv=astro-ph/9510046| postscript=. }} See Table A1, p. 21.</ref>▼
 
<ref name=aaa411_3_559>{{kaynak | display-authors=1| son1=Kovtyukh | ilk1=V. V.| son2=Soubiran | ilk2=C.| son3=Belik | ilk3=S. I.| son4=Gorlova | ilk4=N. I.| başlık=High precision effective temperatures for 181 F-K dwarfs from line-depth ratios | dergi=Astronomy and Astrophysics | cilt=411 | sayı=3 | sayfalar=559–564 |tarih=Aralık 2003 | doi=10.1051/0004-6361:20031378 | arxiv=astro-ph/0308429 | bibcode=2003A&A...411..559K | postscript=. }}</ref>▼
 
<ref name=aaa415>{{kaynak| son1=Santos | ilk1=N. C.| son2=Israelian | ilk2=G.| son3=Mayor | ilk3=M.
| başlık=Spectroscopic <nowiki>[Fe/H]</nowiki> for 98 extra-solar planet-host stars: Exploring the probability of planet formation | dergi=Astronomy and Astrophysics |tarih=Mart 2004 | cilt=415 | sayı=3 | sayfalar=1153–1166 | doi=10.1051/0004-6361:20034469 | arxiv=astro-ph/0311541 | bibcode=2004A&A...415.1153S | postscript=. }}&mdash;the percentage of iron is given by <math>\begin{smallmatrix}10^{-0.13} = 0.74\end{smallmatrix}</math>, or 74%</ref>
 
<ref name=an328_10mnras403_3_1368>{{kaynak| son1=FröhlichGonzalez | ilk1=HG.-E| son2=Carlson | ilk2=M. K.| titleson3=TheTobin differential| ilk3=R. W.| başlık=Parent rotationstars of Epsilonextrasolar Eriplanets from– MOSTX. Lithium abundances and v sini datarevisited | dergi=[[AstronomischeMonthly NachrichtenNotices of the Royal Astronomical Society]] | cilt=328403 | sayı=103 | sayfalar=1037–10391368–1380 |tarih=AralıkNisan 20072010 | doi=10.10021111/asnaj.2007108761365-2966.2009.16195.x | bibcode=2007AN2010MNRAS.403...328.1037F1368G | arxiv=07110912.08061621 | postscript=. }} See table 3.</ref>
 
▲<ref name=aj132_2206>{{kaynak | display-authors=1 | son1=Benedict | ilk1=G. Fritz | son2=McArthur | ilk2=Barbara E. | son3=Gatewood | ilk3=George | son4=Nelan | ilk4=Edmund | son5=Cochran | ilk5=William D. | son6=Hatzes | ilk6=Artie | son7=Endl | ilk7=Michael | son8=Wittenmyer | ilk8=Robert | son9=Baliunas | ilk9=Sallie L.| son10=Walker | ilk10=Gordon A. H. | son11=Yang | ilk11=Stephenson | son12=Kürster | ilk12=Martin | son13=Els | ilk13=Sebastian | son14=Paulson | ilk14=Diane B. |tarih=Kasım 2006 | başlık=The extrasolar planet e Eridani b – orbit and mass | dergi=The Astronomical Journal | cilt=132 | sayı=5 | sayfalar=2206–2218 | bibcode=2006AJ....132.2206B | doi=10.1086/508323 | arxiv=astro-ph/0610247 | postscript=. }}</ref>
 
<ref name=Baines>{{kaynak | son1=Baines| ilk1=Ellyn K. | son2=Armstrong | ilk2=J. Thomas | başlık=Confirming Fundamental Parameters of the Exoplanet Host Star epsilon Eridani Using the Navy Optical Interferometer| dergi=The Astrophysical Journal| cilt=748 | sayfalar=72 | yıl=2011| arxiv=1112.0447 |bibcode = 2012ApJ...748...72B |doi = 10.1088/0004-637X/748/1/72 | postscript=. }}</ref>
 
<ref name="Janson2015"aaa505_1_205>{{kaynak | display-authors=1| son1=JansonDemory | ilk1=MarkusB.-O.| son2=QuanzSégransan | ilk2=Sascha PD. | son3=CarsonForveille | ilk3=Joseph CT. | son4=ThalmannQueloz | ilk4=Christian D.| son5=LafrenièreBeuzit | ilk5=David J.-L.| son6=AmaraDelfosse | ilk6=AdamX.;| son7=di Folco | başlıkilk7=HighE.| son8=Kervella | ilk8=P.| son9=Le Bouquin | ilk9=J.-contrastB.| imagingson10=Perrier with| Spitzer:ilk10=C. deep| observationsson11=Benisty of| Vega,ilk11=M. | son12=Duvert | ilk12=G. | son13=Hofmann | ilk13=K.-H. | son14=Lopez | ilk14=B. | son15=Petrov | ilk15=R. | başlık=Mass-radius relation of Fomalhaut,low and εvery Eridanilow-mass stars revisited with the VLTI | dergi=[[Astronomy &and Astrophysics]] | cilt=574505 | idsayı=A1201 | sayfalartarih=10Ekim 2009 | tarihsayfalar=Şubat 2015205–215 | doi=10.1051/0004-6361/201424944 200911976 | bibcode=2015A2009A&A...574A505.120J.205D | arxiv = 14120906.48160602 | postscript=. }} See Table B.1</ref>
 
<ref name=saaoc8_59an328_10>{{kaynak | son1=CousinsFröhlich | ilk1=AH. W. J-E. | başlıktitle=StandardizationThe differential rotation of BroadbandEpsilon PhotometryEri offrom EquatorialMOST Standardsdata | dergi=South[[Astronomische African Astronomical Observatory CircularsNachrichten]] | cilt=8328 | sayı=5910 | yılsayfalar=19841037–1039 |tarih=Aralık 2007 | doi=10.1002/asna.200710876 | bibcode=1984SAAOC2007AN...8.328.1037F | arxiv=0711.59C0806 | postscript=. }}</ref>
 
▲<ref name=apj460_993>{{kaynak | display-authors=1| son1=Saumon | ilk1=D.| son2=Hubbard | ilk2=W. B.| son3=Burrows | ilk3=A.| son4=Guillot6 | ilk4=T.| son5=Lunine | ilk5=J. I.| son6=Chabrier | ilk6=G.| url=http://articles.adsabs.harvard.edu/full/1996ApJ...460..993S| başlık=A theory of extrasolar giant planets | dergi=The Astrophysical Journal | cilt=460 | sayfa=993 |tarih=Nisan 1996 | doi=10.1086/177027 | bibcode=1996ApJ...460..993S | arxiv=astro-ph/9510046| postscript=. }} See Table A1, p. 21.</ref>
 
▲<ref name=aaa411_3_559>{{kaynak | display-authors=1| son1=Kovtyukh | ilk1=V. V.| son2=Soubiran | ilk2=C.| son3=Belik | ilk3=S. I.| son4=Gorlova | ilk4=N. I.| başlık=High precision effective temperatures for 181 F-K dwarfs from line-depth ratios | dergi=Astronomy and Astrophysics | cilt=411 | sayı=3 | sayfalar=559–564 |tarih=Aralık 2003 | doi=10.1051/0004-6361:20031378 | arxiv=astro-ph/0308429 | bibcode=2003A&A...411..559K | postscript=. }}</ref>
 
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90. satır:
[[Kategori:HIP nesneleri|016537]]
[[Kategori:HR nesneleri|1084]]
[[CategoryKategori:K-tipi ana kol yıldızları]]
[[Kategori:Gezegen sistemleri]]
[[Kategori:Flamsteed cisimleri|Eridani, 18]]
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