• No results found

University of Groningen Cold gas in the center of radio-loud galaxies Maccagni, Filippo

N/A
N/A
Protected

Academic year: 2021

Share "University of Groningen Cold gas in the center of radio-loud galaxies Maccagni, Filippo"

Copied!
2
0
0

Bezig met laden.... (Bekijk nu de volledige tekst)

Hele tekst

(1)

University of Groningen

Cold gas in the center of radio-loud galaxies

Maccagni, Filippo

IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below.

Document Version

Publisher's PDF, also known as Version of record

Publication date: 2017

Link to publication in University of Groningen/UMCG research database

Citation for published version (APA):

Maccagni, F. (2017). Cold gas in the center of radio-loud galaxies: New perspectives on triggering and feedback from HI absorption surveys and molecular gas. Rijksuniversiteit Groningen.

Copyright

Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons).

Take-down policy

If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim.

Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum.

(2)

Stellingen

behorende bij het proefschrift

Cold gas in the centre of radio-loud galaxies

New perspectives on triggering and feedback

from HI absorption surveys and molecular gas

van

Filippo Marcello Maccagni

1. The detection rate of H i absorption in radio galaxies is 27% ± 5.5% and it varies neither with redshift (across the range 0.02 < z < 0.25) nor with radio power (in the range 22.5 <log P1.4 GHz(W Hz−1)< 26.2). (Chapters 1 and 2)

2. Strong interactions between the AGN and the circumnuclear cold gas are likely to occur in compact AGN because the radio jets clear their way through the surrounding medium. (Chapter 1)

3. Broad (FWHM > 200 km s−1) and asymmetric H i absorption lines, which can trace a significant component of gas unsettled by the radio activity, are found only in powerful radio AGN, which have log P1.4 GHz(W Hz−1) > 24 . (Chapters 1 and

2)

4. The kinematics of the H i gas allows to relate the time-scale of formation of the galactic disk to the life cycle of the nuclear activity, and reveal how cold gas can trigger a radio AGN. (Chapter 4)

5. Detecting atomic and molecular hydrogen in AGN in absorption and emission allows to constrain the triggering and fuelling mechanisms of young radio AGN. (Chapters 4, 5 and 6)

6. The absorption by atomic and molecular hydrogen observed in the young radio source PKS B1718–649 traces the fuelling of the AGN in this object. (Chapters 4 and 6)

7. The spark of love is often ignited amongst scientists venturing together on the quest of discovery.

8. Becoming a scientist also means keeping alive the child-like pleasure for knowledge.

9. Nowadays, even if observations are often reduced by automated pipelines, one should never forget to look at the data.

10. History teaches us that it is a mistake to repair the prejudices of the past with new inequities.

Referenties

GERELATEERDE DOCUMENTEN

Since a few of the core prominences of our active sources are comparable to that of the upper limits on the candidate remnants, our results demonstrate that radio-loud AGN with

(2009) divided their SDSS sample into bins cor- responding to di fferent quasar properties: optical luminosity, virial BH mass, quasar color, and radio-loudness.. They found that

The observations suggest a clear 1.25-mm flux density ex- cess over the synchrotron radiation spectrum of MG 1019+0535, suggesting the presence of thermal emission from dust in

( 2017 ) relation agrees well with our inference, which is not surprising since its methods are closest to the assumptions of the H18 models. The infer- ence in this work is

The significant difference in the observed deuterium abundance in PAHs made it desirable to obtain multiple spec- tra of a large number of sources, at a variety of galactic evolu-

High resolution observations of a handful of AGN (e.g. Müller-Sánchez et al. 2016) have characterized the physical conditions (e.g. distribution, kinematics, pressure,

Since it will not be possible to follow up every source where H i is detected in absorption with high resolution observations, MoD_AbS will allow us to relate the properties of the H

If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded