作者: Miguel Sánchez-Portal , Ángeles I. Díaz , Elena Terlevich , Roberto Terlevich
DOI: 10.1111/J.1365-2966.2004.07720.X
关键词: Disc 、 Active galactic nucleus 、 Stellar population 、 Physics 、 Astronomy 、 Emission spectrum 、 Photometry (optics) 、 Bulge 、 Astrophysics 、 Galaxy 、 Luminosity
摘要: We present the results of an investigation on main structural properties derived from VRI and Ha surface photometry galaxies hosting nuclear emission-line regions [including Seyfert 1, 2, low-ionization emission region (LINER) starburst galaxies] as compared with normal galaxies. Our original sample comprises 22 active galaxies, four starbursts one galaxy has been extended several samples obtained literature. Bulge disc parameters, along bulge-to-disc luminosity ratio, have applying iterative procedure. The resulting parameters combined additional data in order to reach a statistically significant sample. find some differences bulge distribution across different types that could imply families bulges physical properties. characteristic colours defined for our control early-type objects. suggest stellar populations are comparable