Hostname: page-component-7479d7b7d-qlrfm Total loading time: 0 Render date: 2024-07-11T02:22:10.709Z Has data issue: false hasContentIssue false
  • English
  • Français

Gamma-rays from massive stars in Cygnus and Orion

Published online by Cambridge University Press:  26 May 2016

Roland Diehl ,
Karsten Kretschmer ,
Stefan Plüschke ,
Miguel Cerviño  and
Dieter H. Hartmann
Roland Diehl
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, D-85741 Garching-bei-Múnchen, BRD
Karsten Kretschmer
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, D-85741 Garching-bei-Múnchen, BRD
Stefan Plüschke
Affiliation:
Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstraße, D-85741 Garching-bei-Múnchen, BRD
Miguel Cerviño
Affiliation:
ESA Laboratorio de Astrofísica Espacial y Física Fundamental (INTA), Apdo. 50727, E-28080 Madrid, España Instituto de Astrofísica de Andalucía (CSIC), Camino Bajo de Huétor 24, E-18080 Granada, España
Dieter H. Hartmann
Affiliation:
Department of Physics and Astronomy, Clemson University, Clemson, SC 29634-0978, USA

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Radioactive 26Al, ejected by massive stars through winds and supernova explosions, leads to γ-ray line emission that can serve as a probe of the interstellar environment in and near young star clusters. The ~ 1 Myr decay time of 26Al is long enough to allow transport over significant distances, which can cause substantial angular offsets between γ-ray emission and cluster stars. Details of such offsets are determined by the morphology of the ISM. We discuss observations in Cygnus and Orion, and models based on population synthesis methods.

Type
Part 4. Feedback from Massive Stars
Information
Symposium - International Astronomical Union , Volume 212: A Massive Star Odyssey: From Main Sequence to Supernova , 2003 , pp. 706 - 709
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Brown, A.G.A., de Geus, E.J., de Zeeuw, P.T. 1994, A&A 289, 101.Google Scholar
Brown, A.G.A., Hartmann, D.H., Burton, W.B. 1995, A&A 300, 903.Google Scholar
Burrows, D.N., Singh, K.P., Nousek, J.A., Garmire, G.P., Good, J. 1993, ApJ 406, 97.Google Scholar
Cerviño, M., Knödlseder, J., Schaerer, D., von Ballmoos, P., Meynet, G. 2000, A&A 363, 970.Google Scholar
Cerviño, M., Valls-Gaboud, D., Luridiana, V., Mas-Hesse, J.M. 2002, A&A 381, 51.Google Scholar
Chen, W., Diehl, R., Gehrels, N., et al. 1997, in: Winkler, C., Courvoisier, T.J.-L. & Durouchoux, Ph. (eds.), The Transparent Universe, Proc. 2nd INTEGRAL Workshop, ESA SP-382, 105.Google Scholar
Diehl, R., Dupraz, C., Bennett, K., et al. 1995, A&A 298, 445.Google Scholar
Diehl, R. 2002, New Astron. Reviews 47, 547.Google Scholar
Heiles, C. 2001, in: Breitschwerdt, D., Freyberg, M.J. & Trümper, J. (eds.), The Local Bubble and Beyond, Lecture Notes in Physics 506, 229.Google Scholar
van der Hucht, K.A. 2001, New Astron. Reviews 45, 135.Google Scholar
de Jager, C., Nieuwenhuijzen, H., van der Hucht, K.A. 1988 A&AS 72, 259.Google Scholar
Knödlseder, J. 1999, ApJ 510, 915.CrossRefGoogle Scholar
Knödlseder, J., Bennett, K., Bloemen, H., et al. 1999, A&A 344, 68.Google Scholar
Knödlseder, J. 2000, A&A 360, 539.Google Scholar
Kretschmer, K. 2000, , .Google Scholar
Meynet, G., Arnould, M., Prantzos, N., Paulus, G. 1997, A&A 320, 460.Google Scholar
Naya, J.E., Barthelmy, S.D., Bartlett, L.M., et al. 1996, Nature 384, 44.Google Scholar
Oberlack, U., Bennett, K., Bloemen, H., et al. 1996, A&AS 120C, 311.Google Scholar
Plüschke, S., Diehl, R., Schönfelder, V., et al. 2000, in: MacConnell, M.L. & Ryan, J.M. (eds.), The Fifth Compton Symposium, AIP-CP 510, 35.Google Scholar
Plüschke, S. 2001, , .Google Scholar
Plüschke, S., Kretschmer, K., Diehl, R., et al. 2001, in: Giménez, A., Reglero, V. & Winkler, C. (eds.), Exploring the Gamma-Ray Universe, Proc. 4th INTEGRAL Workshop, ESA SP-459, 91.Google Scholar
Prantzos, N., Diehl, R. 1996, Physics Reports, 267, 1.Google Scholar
Prinja, R.K., Barlow, M.J., Howarth, I.D. 1990 ApJ 361, 607.Google Scholar
Schaller, G., Schaerer, D., Meynet, G., Maeder, A. 1992, A&AS 96, 269.Google Scholar
Woosley, S.E., Weaver, T. 1995, ApJS 101, 181.CrossRefGoogle Scholar
Woosley, S.E., Langer, N., Weaver, T. 1995, ApJ 448, 315.Google Scholar