Conference Paper
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Photometric and Spectral Analysis of the Open Star Cluster NGC 436

Year 2023, Volume: 4 Issue: 3 - Special Issue: Proceedings of the 22nd National Astronomy Congress, 341 - 348, 31.12.2023
https://doi.org/10.55064/tjaa.1203564

Abstract

In this study, we are aimed to determine the radial velocity and stellar atmospheric parameters such as Teff, logg, [Fe/H] of these stars by using medium resolution spectral data from the LAMOST data archive of some member stars of open star cluster NGC 436. The memberships of the stars were determined from the GAIA EDR3 proper motion data. The GAIA data of the cluster were matched with the UBVRI data from the San Pedro Martir Observatory, and the basic astrophysical parameters of the cluster were examined in many filters. Monte Carlo Markov Chain optimization technique was used in the analysis of spectral data. In addition, the variable types of the stars determined as cluster members were
determined by examining the TESS data.

Supporting Institution

Erciyes Üniversitesi Bilimsel Araştırma Projeler Birimi

Project Number

FDK-2021-11208

Thanks

This research support by the Erciyes Üniversitesi BAP through project number FDK-2021-11208.

References

  • Allende Prietoa C., 2007, The Astronomical Journal, 134, 1843
  • Blanco-Cuaresma S., 2019, Monthly Notices of the Royal Astronomical Society, 486, 2075
  • Blanco-Cuaresma S., Soubiran C., Heiter U., Jofré P., 2014, Astronomy and Astrophysics, 569, 14
  • Bressan A., Marigo P., Girardi L., Salasnich B., Dal Cero C., Rubele S., Nanni A., 2012, Monthly Notices of the Royal Astronomical Society, 427, 127

NGC 436 Açık Yıldız Kümesinin Fotometrik ve Tayfsal Analizi

Year 2023, Volume: 4 Issue: 3 - Special Issue: Proceedings of the 22nd National Astronomy Congress, 341 - 348, 31.12.2023
https://doi.org/10.55064/tjaa.1203564

Abstract

Bu çalışmada, NGC 436 açık yıldız kümesindeki bazı üye yıldızlara ait LAMOST veri arşivinden orta çözünürlükü mevcut tayf verileri kullanılarak bu yıldızlara ait radyal hız ve Teff, logg, [Fe/H] gibi yıldız atmosferik parametrelerinin belirlenmesi amaçlanmıştır. Yıldızların üyelikleri GAIA EDR3 özhareket verilerine göre belirlenmiştir. Kümenin GAIA verileri, San Pedro Martir Gözlemevi’nden alınan UBVRI verileri ile eşleştirilerek kümeye ait temel astrofiziksel parametreler bir çok filtrede incelenmiştir. Tayf verilerinin analizinde Monte Carlo Markov Chain optimizasyon tekniği kullanılmıştır. Ayrıca küme üyesi olarak belirlenen yıldızların TESS verileri incelenerek değişen türleri saptanmıştır.

Project Number

FDK-2021-11208

References

  • Allende Prietoa C., 2007, The Astronomical Journal, 134, 1843
  • Blanco-Cuaresma S., 2019, Monthly Notices of the Royal Astronomical Society, 486, 2075
  • Blanco-Cuaresma S., Soubiran C., Heiter U., Jofré P., 2014, Astronomy and Astrophysics, 569, 14
  • Bressan A., Marigo P., Girardi L., Salasnich B., Dal Cero C., Rubele S., Nanni A., 2012, Monthly Notices of the Royal Astronomical Society, 427, 127
There are 4 citations in total.

Details

Primary Language Turkish
Subjects Astronomical Sciences (Other)
Journal Section Conference Paper
Authors

Yonca Karaca 0000-0003-0893-7298

İnci Akkaya Oralhan 0000-0003-1787-7418

Ahmet Dervişoğlu 0000-0003-1593-1724

Cenk Kayhan 0000-0001-9198-2289

Project Number FDK-2021-11208
Early Pub Date December 18, 2023
Publication Date December 31, 2023
Submission Date November 13, 2022
Acceptance Date January 23, 2023
Published in Issue Year 2023 Volume: 4 Issue: 3 - Special Issue: Proceedings of the 22nd National Astronomy Congress

Cite

TJAA is a publication of Turkish Astronomical Society (TAD).