WebApr 11, 2024 · A spectral line is defined as a dark or bright line in an otherwise continuous and uniform spectrum, resulting from light’s absorption or emission in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used in the identification of molecules and atoms. WebSep 4, 2024 · We estimate a size for the broad-emission-line region, RBELR, of 0.33 pc, derived from the RBELR –luminosity relation 21, and a mass for the black hole, M•, of approximately 2 × 10 10Mʘ from the...
Reverberation mapping - Wikipedia
Webthe continuum and emission line dimming is caused by an increase in dust extinction is disfavored through modeling of the spectral changes. Furthermore, LaMassa et al. (2015) also argue that obscuration by a dust cloud outside the broad-line region in a circular Keplerian orbit is unlikely since its crossing time across the broad-line region ... WebAt least 6 broad-line AGNs (primarily Seyfert 1s) have been detected as well as several narrow-line Seyfert 2 candidates. The Seyfert galaxies detected in our survey have integrated absolute magnitudes extending to M B 𝐵 {}_{B} start_FLOATSUBSCRIPT italic_B end_FLOATSUBSCRIPT ∼ similar-to \sim ∼ -17.5, probing fainter magnitudes and ... knox pools and spas
w264: Emission Line Profiles in AGN - Columbia University
http://www.columbia.edu/~fms5/w264.html http://astro.vaporia.com/start/blr.html WebApr 13, 2024 · Star-forming galaxies that have emission lines with very large EWs at z ≲ 2.5 exhibit tight correlations between the EW of the [O iii] 5007 Å emission line and the O 32 ratio, and between the EWs of [O iii] 5007 Å and Hβ . The properties of the z = 9.51 galaxy are consistent with both of these relations within 2σ (Figure S5). reddit beyond the bump