Öz
Kaynakça
- TJAA cilt 1, sayı 2, s.667–667 (2020) Ulusal Astronomi Kongresi: UAK 2018 – 3 - 7 Eyl ̈ul 2018, Kayseri, Erciyes Universitesi
Öz
We perform multi-wavelength analyses of nearby Seyfert galaxies, which are observed as a part of Local Luminous AGN with Matched Analogues (LLAMA) project. The analyses include UV and optical VLT/X-SHOOTER spectral data of X-ray selected most luminous local Seyfert 1 galaxies. In this study, we aim to obtain SMBH masses by using H$_{\alpha}$ scaling relations and compare our results with M-sigma plane. FWHM results of H$_{\alpha}$ of our sample galaxies are found to be in a wide range (1450 $<$ FWHMH$_{\alpha}$ $<$ 6400 km s-1), which results in a range of black hole masses: 6.3 $<$ log MBH $<$ 7.6 M$_{\odot}$. Resulting BH masses are compared with stellar dispersions, which is measured from CA-Triplet emission line. In our preliminary results, we conclude that the majority of our Seyfert 1 galaxies host disk-like bulges, namely pseudo-bulges.
Anahtar Kelimeler
Kaynakça
- TJAA cilt 1, sayı 2, s.667–667 (2020) Ulusal Astronomi Kongresi: UAK 2018 – 3 - 7 Eyl ̈ul 2018, Kayseri, Erciyes Universitesi
Ayrıntılar
| Birincil Dil | İngilizce |
|---|---|
| Konular | Astronomik Bilimler (Diğer) |
| Bölüm | Bildiri |
| Yazarlar | |
| Yayımlanma Tarihi | 11 Aralık 2020 |
| Gönderilme Tarihi | 19 Şubat 2019 |
| Kabul Tarihi | 3 Eylül 2019 |
| Yayımlandığı Sayı | Yıl 2020 Cilt: 1 Sayı: 2 |
TJAA, Türk Astronomi Derneğinin (TAD) bir yayınıdır.