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galaxies: Seyfert

Very high energy gamma-ray emission of NGC 1275 and 3c382 and the possible activity nature of the Seyfert Galaxies

Very high energy gamma-ray emission of NGC 1275 and 3c382 and the possible activity nature of the Seyfert Galaxies

... Galaxy clusters have been consider as sources of TeV γ- rays emitted by high-energy protons and electrons accel- erated by large scale structure formation shocks, galactic winds, or active galactic nuclei. The Perseus ...

5

On the Extent of the Existence of Broad Line Region in Seyfert Galaxies

On the Extent of the Existence of Broad Line Region in Seyfert Galaxies

... in Seyfert galaxies that produce the strong radiation which excites gas around the central regions, giving rise to the observed emission lines ...of Seyfert galaxies comes either from the ...

6

Properties of the Narrow Line Seyfert 1  Galaxies Revisited

Properties of the Narrow Line Seyfert 1 Galaxies Revisited

... of Seyfert galaxies and low luminosity AGN in [33] whose disk luminosity is mostly less than 10 44 erg/s, and the correlation index between the jet power and disk luminosity is steeper in the RL-NLS1s than ...

9

Continuum reverberation mapping of the accretion disks in two Seyfert 1 galaxies

Continuum reverberation mapping of the accretion disks in two Seyfert 1 galaxies

... We present optical continuum lags for two Seyfert 1 galaxies, MCG + 08-11-011 and NGC 2617, using monitoring data from a reverberation mapping campaign carried out in 2014. Our light curves span the ugriz fi ...

20

A panchromatic view of relativistic jets in narrow-line Seyfert 1 galaxies

A panchromatic view of relativistic jets in narrow-line Seyfert 1 galaxies

... narrow-line Seyfert 1 (NLSy1) galaxies revealed the presence of a possible third class of AGN with relativistic jets in addition to blazars and radio ...spiral galaxies, this finding poses intriguing ...

11

A radio and infrared investigation of Seyfert galaxies in the local universe

A radio and infrared investigation of Seyfert galaxies in the local universe

... Lawrence (1987) is a thorough, early review of AGN unification in general. There have been several, slightly differing (in most cases) models (Blanford & Königl 1979; Wilson 1981, 1982; Pedlar et al. 1985; Wilson ...

197

Lin, Ming-Yi
  

(2017):


	Gas flows and stars in nuclear regions of nearby seyfert galaxies.


Dissertation, LMU München: Fakultät für Physik

Lin, Ming-Yi (2017): Gas flows and stars in nuclear regions of nearby seyfert galaxies. Dissertation, LMU München: Fakultät für Physik

... the Seyfert galaxies in the combined sample summarised in Table ...two galaxies could also be used for this analysis, we have not included them ...

145

Relativistic jets in narrow-line Seyfert 1 galaxies. New discoveries and open questions

Relativistic jets in narrow-line Seyfert 1 galaxies. New discoveries and open questions

... Before the launch of the Fermi satellite only two classes of AGNs were known to produce these structures and thus to emit up to the γ-ray energy range: blazars and radio galaxies, both hosted in giant elliptical ...

6

Velocity resolved reverberation mapping of five bright Seyfert 1 galaxies

Velocity resolved reverberation mapping of five bright Seyfert 1 galaxies

... The scaling factor f can be determined for an AGN if there is an independent measurement of the black hole mass. Unfortunately, there are few cases where the black hole radius of influence is large enough that either ...

32

X-ray Evolution and Variability of Active Galactic Nuclei

X-ray Evolution and Variability of Active Galactic Nuclei

... a Seyfert 1 type of spectrum is observed) but when viewed edge on th e broad line region is obscured by the m olecular torus and only the narrow lines are visible ...a Seyfert 2 type of spectrum ...

206

Trojans in Wireless Sensor Networks

Trojans in Wireless Sensor Networks

... typically Seyfert-like galaxies, with the initial assumption being that those objects that demonstrated the greatest g -ray emission and/or radio loudness would also show the most blazar-like ...and ...

434

GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024 0+1652 at z=0 395

GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster ZwCl 0024 0+1652 at z=0 395

... We have explored the available mechanisms for separating the population of SF galaxies and AGNs. Broad-line AGNs (BLAGN) show permitted lines with widths of thousands of kilometres per second. By contrast, in ...

22

SDSS IV MaNGA   the spatially resolved transition from star formation to quiescence

SDSS IV MaNGA the spatially resolved transition from star formation to quiescence

... that galaxies with more massive bulges experience a larger amount of energetic feedback from their black ...(including Seyfert galaxies and quasars) and radio- mode ...of galaxies (inner few ...

20

Astronomy   Galaxies and the Expanding Universe pdf

Astronomy Galaxies and the Expanding Universe pdf

... active galaxies, such as Seyfert galaxies, originally recognized by the American astronomer Carl ...K. Seyfert from optical spectra. Seyfert galaxies have very bright nuclei with ...

227

School Desegregation, Law and Order, and Litigating Social Justice in Alabama, 1954 1973

School Desegregation, Law and Order, and Litigating Social Justice in Alabama, 1954 1973

... One of the the primary motivations of the work presented in this dissertation is to compare the properties of RL NLS1 galaxies to those of blazars. In order to achieve this, the various prop- erties measured for ...

298

Queer Feelings, Political Potential: Tracing Affect in Performance Spaces

Queer Feelings, Political Potential: Tracing Affect in Performance Spaces

... Active Galactic Nuclei (AGN) are axisymmetric systems to first order; their observed prop- erties are likely strong functions of inclination with respect to our line of sight. However, except for a few special cases, the ...

214

Determining the halo mass scale where galaxies lose their gas

Determining the halo mass scale where galaxies lose their gas

... cluster galaxies, they found that the fi eld galaxies were approximately 1 – 2 Gyr younger than the cluster galaxies at a fi xed stellar ...eld galaxies and explore the consequences ...old ...

22

Triggering active galactic nuclei in galaxy clusters

Triggering active galactic nuclei in galaxy clusters

... of galaxies It is important to note that the distribution of AGN in the phase space as shown in ...from galaxies that have a distribution in clustercentric radius and mass that matches that of the Pimbblet ...

14

Chemical evolution of star-forming galaxies in the overdense environment

Chemical evolution of star-forming galaxies in the overdense environment

... of galaxies in the cluster environ- ...cluster galaxies, giving direct evidence of RPS in cluster environments (Abramson et ...cluster galaxies are HI deficient compared to field galaxies and ...

146

nIFTy cosmology: comparison of galaxy formation models

nIFTy cosmology: comparison of galaxy formation models

... of galaxies from their halo mass distribution, but modelling choices and choices of which constraints to use re- sult in different models having different predictions for relations between galaxies and ...

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