Analogo solare: differenze tra le versioni

Versione delle 16:17, 18 ott 2021

Versione delle 16:24, 18 ott 2021

Riga 534:

| 175

| G2V

| 5,783 773

|style="background-color:Moccasin;"| 5 773

| -0,06

| 3,9

|<ref name="Galarza">{{citaCita pubblicazione|url=http://www.aanda.org/articles/aa/pdf/2014/03/aa22277-13.pdf|titolo=AExplosive photometricnucleosynthesis andof spectroscopica metal-deficient star as the surveysource of a distinct odd-even effect in the solar twin starsHIP within11915|autore=Jhon 50Yana Galarza|etal=si|rivista=[[Monthly parsecsNotices of the Sun|rivista=AstronomyRoyal &Astronomical AstrophysicsSociety]]|volume=563502|numero= A521|data=2014Marzo 2021|doiarxiv=102101.1051/0004-6361/20132227710182}}</ref>

|-

|style="text-align:left;"| [[HD 101364]]

| {{RA|11|40|28.5}}

| {{DEC|+69|00|31}}

| 217

| G5V

| 5.4 783

| +0.,01

| 5,7804

|<ref name=apj669_2/><ref name=vazquez_et_al_2010>{{cita libro | autore=Vázquez, M.; Pallé, E.; Rodríguez, P. Montañés |capitolo=Is Our Environment Special? | anno=2010 | pagine=391–418 | titolo=The Earth as a Distant Planet: A Rosetta Stone for the Search of Earth-Like Worlds | serie=Astronomy and Astrophysics Library | editore=Springer New York | doi=10.1007/978-1-4419-1684-6 | isbn=978-1-4419-1683-9 }}</ref>

|-

|style="text-align:left;"| [[YBP 1194]]

| {{RA|08|51|00.807}}

| {{DEC|+11|48|52.76}}

| 2772

| G5V

| 5,675 780

| +0.,023

| 4.,2

|<ref>{{cita pubblicazione|autore= A. Önehag ''et al.'' | url= http://www.aanda.org/articles/aa/pdf/2011/04/aa15138-10.pdf|titolo= M67-1194, an unusually Sun-like solar twin in M67|rivista= [[Astronomy & Astrophysics]]|volume=528|numero=A85|pagina=11 |data=aprile 2011|doi=10.1051/0004-6361/201015138}}</ref>

|-

|style="text-align:left;"| [[HD 186302]]

| {{RA|19|49|06.43}}

| {{DEC|-70|11|16.70}}

| 184,11

| G3/G5V

| 5 675

| +0.,00

| 4.,5

|<ref name="Adibekyan"> {{cita pubblicazione| url=https://www.aanda.org/articles/aa/full_html/2018/11/aa34285-18/aa34285-18.html | autore=V. Adibekyan (Վարդան Ադիբեկյան) ''et al.'' | titolo=The AMBRE project: searching for the closest solar siblings | rivista=[[Astronomy_and_Astrophysics|Astronomy & Astrophysics]] | volume=619 | numero=Nov | anno=2018 | p=19 | doi=10.1051/0004-6361/201834285 }}</ref>

|-

Riga 553 ⟶ 584:

| {{RA|16|15|37.3}}

| {{DEC|–08|22|06}}

| 45.,1

| G2Va

|style="background-color:Moccasin;"| 5 835

Riga 575 ⟶ 606:

| 92

| G5

| 5, 760

| -0.,04

| 5.,1

|<ref name="Takeda">{{cita pubblicazione | autore=Takeda, Y.; Tajitsu, A. | titolo=High-Dispersion Spectroscopic Study of Solar Twins: HIP 56948, HIP 79672, and HIP 100963 | rivista=Publications of the Astronomical Society of Japan | anno=2009 | arxiv=0901.2509T| volume=61 | pagine=471 }}</ref>

Riga 586 ⟶ 617:

| 101

| G5IV-V

| 5, 710

| –0.,03

|style="background-color:Moccasin;"| 7.,8

|<ref name=apj130_5>{{cita pubblicazione | autore=King, Jeremy R.; Boesgaard, Ann M.; Schuler, Simon C. | titolo=Keck HIRES Spectroscopy of Four Candidate Solar Twins | rivista=The Astronomical Journal | volume=130 | pagine=2318–2325 | mese=novembre| anno=2005 | doi=10.1086/452640}}{{arxiv|astro-ph|0508004}}</ref>

|-

Riga 596 ⟶ 627:

| 103

| G2V

|style="background-color:Moccasin;"| 5, 841

|style="background-color:Moccasin;"| –0.,15

| 5.,0

|<ref name=apj130_5/>

|-

Riga 606 ⟶ 637:

| 126

| G5V

|style="background-color:Moccasin;"| 5, 851

| +0.,03

| 4.,7

|<ref name=apj669_2/>

|-

Riga 616 ⟶ 647:

| 141

| G0

| 5, 768

| +0.,00

| 3.,8

|<ref name=apj130_5/>

|-

Riga 626 ⟶ 657:

| 154

| G2V

| 5, 749

| –0.,02

|style="background-color:Moccasin;"| 8.,2

|<ref name=apj130_5/>

|-

Riga 636 ⟶ 667:

| 171

| G0

| 5, 808

| +0.,02

|style="background-color:Moccasin;"| 6.,3

|<ref name=apj669_2/>

|-

|style="text-align:left;"| [[HD 101364]]

| {{RA|11|40|28.5}}

| {{DEC|+69|00|31}}

| 217

| G5V

| 5,783

| +0.01

| 5.4

|<ref name=apj669_2/><ref name=vazquez_et_al_2010>{{cita libro | autore=Vázquez, M.; Pallé, E.; Rodríguez, P. Montañés |capitolo=Is Our Environment Special? | anno=2010 | pagine=391–418 | titolo=The Earth as a Distant Planet: A Rosetta Stone for the Search of Earth-Like Worlds | serie=Astronomy and Astrophysics Library | editore=Springer New York | doi=10.1007/978-1-4419-1684-6 | isbn=978-1-4419-1683-9 }}</ref>

|-

|style="text-align:left;"| [[YBP 1194]]

| {{RA|08|51|00.807}}

| {{DEC|+11|48|52.76}}

| 2772

| G5V

| 5,780

| +0.023

| 4.2

|<ref>{{cita pubblicazione|autore= A. Önehag ''et al.'' | url= http://www.aanda.org/articles/aa/pdf/2011/04/aa15138-10.pdf|titolo= M67-1194, an unusually Sun-like solar twin in M67|rivista= [[Astronomy & Astrophysics]]|volume=528|numero=A85|pagina=11 |data=aprile 2011|doi=10.1051/0004-6361/201015138}}</ref>

|-

|style="text-align:left;"| [[HD 186302]]

| {{RA|19|49|06.43}}

| {{DEC|-70|11|16.70}}

| 184,11

| G3/G5V

| 5,675

| +0.00

| 4.5

|<ref name="Adibekyan"> {{cita pubblicazione| url=https://www.aanda.org/articles/aa/full_html/2018/11/aa34285-18/aa34285-18.html | autore=V. Adibekyan (Վարդան Ադիբեկյան) ''et al.'' | titolo=The AMBRE project: searching for the closest solar siblings | rivista=[[Astronomy_and_Astrophysics|Astronomy & Astrophysics]] | volume=619 | numero=Nov | anno=2018 | p=19 | doi=10.1051/0004-6361/201834285 }}</ref>

|}