Probing the Strong (Stationary) Gravitational Field of Accreting Black Holes with X-ray Observations
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy
Link
http://link.springer.com/article/10.1007/s10701-018-0212-x/fulltext.html
Reference48 articles.
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2. Bambi, C.: Probing the space-time geometry around black hole candidates with the resonance models for high-frequency QPOs and comparison with the continuum-fitting method. JCAP 9, 014 (2012). https://doi.org/10.1088/1475-7516/2012/09/014
3. Bambi, C.: Measuring the Kerr spin parameter of a non-Kerr compact object with the continuum-fitting and the iron line methods. JCAP 8, 055 (2013). https://doi.org/10.1088/1475-7516/2013/08/055
4. Belloni, T.M., Stella, L.: Fast variability from black-hole binaries. Space Sci. Rev. 183, 43–60 (2014). https://doi.org/10.1007/s11214-014-0076-0
5. de La Calle Pérez, I., Longinotti, A.L., Guainazzi, M., Bianchi, S., Dovčiak, M., Cappi, M., Matt, G., Miniutti, G., Petrucci, P.O., Piconcelli, E., Ponti, G., Porquet, D., Santos-Lleó, M.: FERO: finding extreme relativistic objects. I. Statistics of relativistic $$\text{ Fe } \text{ K }_{\alpha }$$ Fe K α lines in radio-quiet Type 1 AGN. Astron. Astrophys. 524, A50 (2010). https://doi.org/10.1051/0004-6361/200913798
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