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A starburst region around l = 347° − 350°

Published online by Cambridge University Press:  31 March 2017

A. Marco
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal. Escuela Politécnica Superior. University of Alicante. Apdo.99 E-03080. Alicante, Spain email: [email protected]
I. Negueruela
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal. Escuela Politécnica Superior. University of Alicante. Apdo.99 E-03080. Alicante, Spain email: [email protected]
M. Monguió
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal. Escuela Politécnica Superior. University of Alicante. Apdo.99 E-03080. Alicante, Spain email: [email protected]
C. González-Fernández
Affiliation:
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, United Kingdom
J. Maíz Apellániz
Affiliation:
Centro de Astrobiología, CSIC-INTA, campus ESAC, apartado postal 78, 28 691 Villanueva de la Cañada, Madrid, Spain
R. Dorda
Affiliation:
Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal. Escuela Politécnica Superior. University of Alicante. Apdo.99 E-03080. Alicante, Spain email: [email protected]
J. S. Clark
Affiliation:
Department of Physics and Astronomy, The Open University, Walton Hall, Milton Keynes, MK7 6AA, United Kingdom
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Abstract

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Very recently, a number of obscured massive open clusters have been identified in the Milky Way. A very significant fraction of them lie either close to the base of the Scutum Arm or towards Galactic longitude of 350°. We are studying these clusters and their neighbourhoods, finding very good evidence for a major starburst region close to the near tip of the Galactic Long Bar.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2017 

References

Marco, A., Negueruela, I., González-Fernández, C., et al. 2014 A&A, 567, A73 Google Scholar
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