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Gemini 3D infrared spectroscopy: Double nucleus in M 83

Published online by Cambridge University Press:  24 November 2004

Rubén J. Díaz
Affiliation:
Observatorio Astronómico de Córdoba, Córdoba, Argentina e-mail: [email protected]
María P. Agüero
Affiliation:
Observatorio Astronómico de Córdoba, Córdoba, Argentina e-mail: [email protected] SeCyT, Universidad Nacional de Córdoba, Argentina
Horacio Dottori
Affiliation:
Instituto de Física, Universidade Federal do Rio Grande do Sul, Porto Alegre, Brazil
Damián Mast
Affiliation:
Observatorio Astronómico de Córdoba, Córdoba, Argentina e-mail: [email protected] SeCyT, Universidad Nacional de Córdoba, Argentina
Gustavo Carranza
Affiliation:
Observatorio Astronómico de Córdoba, Córdoba, Argentina e-mail: [email protected] CONICET, Argentina
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Abstract

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We report the status of our study of the central region of M 83. Recently a binary mass concentration at the nucleus was suggested by Thatte et al. (2000), and we determined the possible position of the optically hidden mass concentration with 2D Hα kinematics. We continue our study of this region trough IR 3D spectroscopy performed with CIRPASS, attached to the Gemini South telescope. Almost 1500 spectra were obtained, centered in the wavelength 1.3 μm. The velocity field in a region of 13″ × 9″ around the optical nucleus is resolved, with 0.36″ (6.4 pc) sampling. We confirm that the optical nucleus of M 83 is not located at the most important center of symmetry of the velocity field. The largest black hole that could fit to the circular motion in this kinematic center should have a mass less than $2\times10^7M_{\odot}$.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
POSTERS
Copyright
© 2004 International Astronomical Union