Bu çalışmada ötegezegen barındıran HAT-P-19 yıldızının yüksek çözünürlüklü (R = 55000)KECK/HIRES tayfı tekrar analiz edilip temel atmosfer parametreleri ve bazı elementlerin bolluğu hesaplanmıştır.
Albrecht, S., vd.: Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments. AJ. 757 (2012) 18
Asplund, M., vd.: The Chemical Composition of the Sun. ARA&A. 47 (2009) 481--522
Blanco-Cuaresma, S., Soubiran, C., Heiter, U., Jofre, P.: iSpec: Stellar atmospheric parameters and chemical abundances. ASCL (2014) record ascl:1409.006
Brewer, M., vd.: pectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-search Stars. APJ. 225 (2016) 36
Buchhave, A., vd.: An abundance of small exoplanets around stars with a wide range of metallicities. Nature. 486 (2012) 375--377
Castelli, F., Kurucz, R. L., : New Grids of ATLAS9 Model Atmospheres. (2004) arXiv:astro-ph/0405087
Girardi, L., vd.: Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 Msun, and from Z=0.0004 to 0.03. A&AS. bf 141 (2000) 371--383
Guillot, T., vd.: A correlation between the heavy element content of transiting extrasolar planets and the metallicity of their parent stars. A&A. 453 (2006) 21--24
Hartman, J. D., vd.: HAT-P-18b and HAT-P-19b: Two Low-density Saturn-mass Planets Transiting Metal-rich K Stars. APJ. 726 (2011) 16
Hinkel, N., vd.: A Recommendation Algorithm to Predict Giant Exoplanet Host Stars Using Stellar Elemental Abundances. (2018) arXiv:1805.12144
Kurucz, L.: SYNTHE spectrum synthesis programs and line data. SAO (1993)
Piskunov, Nikolai & Kupka, F & A. Ryabchikova, T & Weiss, Werner & Jeffery, Simon.: VALD: The Vienna Atomic Line Data Base. A&ASS 112 (1995) 525
Santos, N., Israelian, G., Mayor, M.: Spectroscopic [Fe/H] for 98 extra-solar planet-host stars. Exploring the probability of planet formation. A&A. 415 (2004) 1153--1166
Sneden, C. vd.: MOOG: LTE line analysis and spectrum synthesis. ASCL (2012) record ascl:1202.009
Sozzetti, A., vd.:When Do Planets Form? A Search for Extra-solar Planets around Metal-Poor Stars. Extrasolar Planets: Today and Tomorrow, ASP Conference Proceedings. 321 (2004) 30
Tsantaki, M., vd.: Deriving precise parameters for cool solar-type stars. Optimizing the iron line list. A&A. 555 (2013) 11
Winn, J. vd.: Hot Stars with Hot Jupiters Have High Obliquities. AJL. 718 (2010) 145--149
Valenti, A., Piskunov, N. E.: Spectroscopy Made Easy. MASS 108 (1996)
Albrecht, S., vd.: Obliquities of Hot Jupiter Host Stars: Evidence for Tidal Interactions and Primordial Misalignments. AJ. 757 (2012) 18
Asplund, M., vd.: The Chemical Composition of the Sun. ARA&A. 47 (2009) 481--522
Blanco-Cuaresma, S., Soubiran, C., Heiter, U., Jofre, P.: iSpec: Stellar atmospheric parameters and chemical abundances. ASCL (2014) record ascl:1409.006
Brewer, M., vd.: pectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-search Stars. APJ. 225 (2016) 36
Buchhave, A., vd.: An abundance of small exoplanets around stars with a wide range of metallicities. Nature. 486 (2012) 375--377
Castelli, F., Kurucz, R. L., : New Grids of ATLAS9 Model Atmospheres. (2004) arXiv:astro-ph/0405087
Girardi, L., vd.: Evolutionary tracks and isochrones for low- and intermediate-mass stars: From 0.15 to 7 Msun, and from Z=0.0004 to 0.03. A&AS. bf 141 (2000) 371--383
Guillot, T., vd.: A correlation between the heavy element content of transiting extrasolar planets and the metallicity of their parent stars. A&A. 453 (2006) 21--24
Hartman, J. D., vd.: HAT-P-18b and HAT-P-19b: Two Low-density Saturn-mass Planets Transiting Metal-rich K Stars. APJ. 726 (2011) 16
Hinkel, N., vd.: A Recommendation Algorithm to Predict Giant Exoplanet Host Stars Using Stellar Elemental Abundances. (2018) arXiv:1805.12144
Kurucz, L.: SYNTHE spectrum synthesis programs and line data. SAO (1993)
Piskunov, Nikolai & Kupka, F & A. Ryabchikova, T & Weiss, Werner & Jeffery, Simon.: VALD: The Vienna Atomic Line Data Base. A&ASS 112 (1995) 525
Santos, N., Israelian, G., Mayor, M.: Spectroscopic [Fe/H] for 98 extra-solar planet-host stars. Exploring the probability of planet formation. A&A. 415 (2004) 1153--1166
Sneden, C. vd.: MOOG: LTE line analysis and spectrum synthesis. ASCL (2012) record ascl:1202.009
Sozzetti, A., vd.:When Do Planets Form? A Search for Extra-solar Planets around Metal-Poor Stars. Extrasolar Planets: Today and Tomorrow, ASP Conference Proceedings. 321 (2004) 30
Tsantaki, M., vd.: Deriving precise parameters for cool solar-type stars. Optimizing the iron line list. A&A. 555 (2013) 11
Winn, J. vd.: Hot Stars with Hot Jupiters Have High Obliquities. AJL. 718 (2010) 145--149
Valenti, A., Piskunov, N. E.: Spectroscopy Made Easy. MASS 108 (1996)
Toplam 18 adet kaynakça vardır.
Ayrıntılar
Birincil Dil
Türkçe
Konular
Astronomik Bilimler (Diğer)
Bölüm
Bildiri
Yazarlar
Selçuk Yalçınkaya
Türkiye
Özgür Baştürk
ANKARA ÜNİVERSİTESİ, FEN FAKÜLTESİ, ASTRONOMİ VE UZAY BİLİMLERİ BÖLÜMÜTürkiye