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Gamma-ray emitting narrow-line Seyfert 1 galaxies. New discoveries and open questions

Published online by Cambridge University Press:  25 July 2014

F. D'Ammando*
Affiliation:
INAF - Istituto di Radioastronomia, Via Gobetti 101, I-40129 Bologna, Italy
M. Orienti
Affiliation:
INAF - Istituto di Radioastronomia, Via Gobetti 101, I-40129 Bologna, Italy
J. Finke
Affiliation:
U.S. Naval Research Laboratory, 4555 Overlook Ave. SW, Washington, DC 20375-5352, USA
J. Larsson
Affiliation:
KTH, Dep. of Physics, and the Oskar Klein Centre, AlbaNova, SE-106 91 Stockholm, Sweden
M. Giroletti
Affiliation:
INAF - Istituto di Radioastronomia, Via Gobetti 101, I-40129 Bologna, Italy
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Abstract

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The discovery of γ-ray emission from 5 radio-loud narrow-line Seyfert 1 galaxies revealed the presence of a possible emerging third class of AGNs with relativistic jets, in addition to blazars and radio galaxies. The existence of relativistic jets also in this subclass of Seyfert galaxies opened an unexplored research space for our knowledge of the radio-loud AGNs. Here, we discuss the radio-to-γ-rays properties of the γ-ray emitting narrow-line Seyfert 1 galaxies, also in comparison with the blazar scenario.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2014 

References

Abdo, A. A., Ackermann, M., Ajello, M., et al. 2009, ApJ, 707, L142CrossRefGoogle Scholar
Abdo, A. A., Ackermann, M., Ajello, M., et al. 2010, ApJ, 710, 1271Google Scholar
Ackermann, M., Ajello, M., Allafort, A., et al. 2012, ApJ, 747, 104Google Scholar
Anton, S., Browne, I. W. A., & Marcha, M. J. 2008, A&A, 490, 583Google Scholar
Böttcher, M. & Dermer, C. D. 2002, ApJ, 564, 86Google Scholar
Blandford, R. D. & Rees, M. J. 1978, in BL Lac Objects ed. A. M. Wolfe, 328Google Scholar
Calderone, G., Ghisellini, G., Colpi, M., & Dotti, M. 2013, MNRAS, 431, 210Google Scholar
Carpenter, B. & Ojha, R. 2013, The Astronomer's Telegram, 5344, 1Google Scholar
Chatterjee, R., Fossati, G., Urry, C. M., et al. 2013, ApJ, 763, L11Google Scholar
D'Ammando, F., Raiteri, C. M., Villata, M., et al. 2011, A&A, 529, 145Google Scholar
D'Ammando, F., Orienti, M., Finke, J., et al. 2012, MNRAS, 426, 317Google Scholar
D'Ammando, F., Orienti, M., Doi, A., et al. 2013a, MNRAS, 433, 952Google Scholar
D'Ammando, F., Tosti, G., Orienti, M., & Finke, J. 2013b, 2012 Fermi Symposium proceedingsGoogle Scholar
D'Ammando, F., Carpenter, B., & Ojha, R. 2013c, The Astronomer's Telegram, 5352, 1Google Scholar
D'Ammando, F., Larsson, J., Orienti, M., et al. 2014, MNRAS, 438, 3521Google Scholar
D'Ammando, F., Orienti, M., Finke, J., et al. 2013d, MNRAS, 436, 191Google Scholar
Foschini, L., Ghisellini, G., Kovalev, Y. Y., et al. 2011, MNRAS, 413, 1671CrossRefGoogle Scholar
Foschini, L., Angelakis, E., Fuhrmann, L., et al. 2012, A&A, 548, A106Google Scholar
Giroletti, M., Paragi, Z., Bignall, H., et al. 2011, A&A, 528, L11Google Scholar
Grupe, D., Komossa, S., Leighly, K. M., & Page, K. L. 2010, ApJS, 187, 64CrossRefGoogle Scholar
Komossa, S., Voges, W., Xu, D., et al. 2006, AJ, 132, 531Google Scholar
Marconi, A., Axon, D. J., Maiolino, R., et al. 2008, ApJ, 678, 693Google Scholar
Marscher, A. 2009, in Lecture Notes in Physics 794, ed. T. Belloni, 173Google Scholar
Nolan, P., Abdo, A. A., Ackermann, M., et al. 2012, ApJS, 199, 31Google Scholar
Osterbrock, D. E. & Pogge, R. W. 1985, ApJ, 297, 166CrossRefGoogle Scholar
Pogge, R. W. 2000, New Astron. Revs, 44, 381Google Scholar
Sikora, M., Stawarz, L., & Lasota, J.-P. 2007, ApJ, 658, 815Google Scholar
Sikora, M. 2009, AN, 330, 291Google Scholar
Yuan, W., Zhou, H.-Y., Komossa, S., et al. 2008, ApJ, 685, 801Google Scholar
Zhou, H.-Y., Wang, T.-G., Yuan, W., et al. 2006, ApJS, 166, 128Google Scholar