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The Close AGN Reference Survey (CARS). What is causing Mrk 1018ś return to the shadows after 30 years?

MPS-Authors

Husemann,  B.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Urrutia,  T.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Tremblay,  G.R.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Krumpe,  M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Dexter,  J.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Busch,  G.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Combes,  F.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Croom,  S.M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Davis,  T.A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Eckart,  A.
Max Planck Institute for Radio Astronomy, Max Planck Society;

McElroy,  R.E.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Perez-Torres,  M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Powell,  M.
Max Planck Institute for Radio Astronomy, Max Planck Society;

Scharwächter, 
Max Planck Institute for Radio Astronomy, Max Planck Society;

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Citation

Husemann, B., Urrutia, T., Tremblay, G., Krumpe, M., Dexter, J., Busch, G., et al. (2016). The Close AGN Reference Survey (CARS). What is causing Mrk 1018ś return to the shadows after 30 years? Astronomy and Astrophysics, 593: L9, pp. L9. doi:10.1051/0004-6361/201629245.


Cite as: http://hdl.handle.net/11858/00-001M-0000-002E-1530-3
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