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A starburst region around l = 347° − 350°

Published online by Cambridge University Press:  31 March 2017

A. Marco ,
I. Negueruela ,
M. Monguió ,
C. González-Fernández ,
J. Maíz Apellániz ,
R. Dorda  and
J. S. Clark
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: amparo.marco@ua.es
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: amparo.marco@ua.es
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: amparo.marco@ua.es
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: amparo.marco@ua.es
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.

Keywords

open cluster and associations:VdBH 222 and Teutsch 85supergiantGalactic structure
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 165 - 166
Copyright
Copyright © International Astronomical Union 2017 

References

Marco, A., Negueruela, I., González-Fernández, C., et al. 2014 A&A, 567, A73 Google Scholar
Eggenberger, P., Meynet, G., & Maeder, A. 2002, A&A, 386, 576 Google Scholar
Zhang, B., Moscadelli, L., & Sato, M., Reid, M. J., et al. 2014, ApJ, 781, A89 Google Scholar
Negueruela, I., González-Fernández, C.; Marco, A., & Clark, J. S. 2011, A&A, 528, A59 Google Scholar
Negueruela, I., Marco, A., González-Fernández, C., et al. 2012 A&A, 547, A15 Google Scholar
González-Fernández, C. & Negueruela, I. 2012 A&A, 539, A100 Google Scholar