Hostname: page-component-78c5997874-m6dg7 Total loading time: 0 Render date: 2024-11-07T07:21:45.034Z Has data issue: false hasContentIssue false
  • English
  • Français

Theory and Models of the Disk-Halo Connection

Modelling the Disk-Halo Interaction in Galaxies

Published online by Cambridge University Press:  17 September 2012

D. Breitschwerdt ,
M.A. de Avillez ,
V. Baumgartner  and
V.A. Dogiel
D. Breitschwerdt
Affiliation:
Zentrum für Astronomie und Astrophysik, Technische Universität Berlin, Hardenbergstr. 36, 0623 Berlin, Germany
M.A. de Avillez
Affiliation:
Department of Mathematics, University of Évora, R. Romão Ramalho 59, 7000 Évora, Portugal
V. Baumgartner
Affiliation:
Institut für Astronomie, University of Vienna, Türkenschanzstr. 17, 1180 Vienna, Austria
V.A. Dogiel
Affiliation:
P.N. Lebedev Institute, Leninskii pr, 53, 119991 Moscow, Russia
Get access

Abstract

We review the evolution of the interstellar medium in disk galaxies, and show, both analytically and by numerical 3D hydrodynamic simulations, that the disk-halo connection is an essential ingredient in understanding the evolution of star forming galaxies. Depending on the star formation rate of the underlying gaseous disk, a galactic fountain is established. If the star formation rate is sufficiently high and/or cosmic rays are well coupled to the thermal plasma, a galactic wind will be formed and lead to a secular mass loss of the galaxy. Such a wind leaves a unique imprint on the soft X-ray spectra in edge-on galaxies, with delayed recombination being one of its distinctive features. We argue that synthetic spectra, obtained from self-consistent dynamical and thermal modeling of a galactic outflow, should be treated on an equal footing as observed spectra. We show that it is thus possible to successfully fit the spectrum of the starburst galaxy NGC 3079

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 56: The Role of the Disk-Halo Interaction in Galaxy Evolution: Outflow vs. Infall? , 2012 , pp. 333 - 342
Copyright
© EAS, EDP Sciences, 2012

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Anders, E., & Grevesse, N., 1989, GeCoA, 53, 197CrossRef
Avillez, M.A., 2000, MNRAS, 315, 479CrossRef
Avillez, M.A., & Breitschwerdt, D., 2004, A&A, 425, 899
Avillez, M.A., & Breitschwerdt, D., 2005, A&A, 436, 585
Basu, S., Johstone, D. & Martin, P.G., 1999, ApJ, 516, 843CrossRef
Baumgartner, V., 2007, Master’s Thesis, University of Vienna, 121Google Scholar
Berghöfer, T., & Breitschwerdt, D., 2002, A&A, 390, 299
Bisnovatyi-Kogan, G.S., & Silich, S.A., 1995, RvMP, 67, 661
Bregman, J.N., 1980, ApJ, 236, 577CrossRef
Bregman, J.N., & Houck, J.C., 1997, ApJ, 485, 159CrossRef
Breitschwerdt, D., McKenzie, J.F., & Völk, H.J., 1991, A&A, 245, 79
Breitschwerdt, D., & Schmutzler, T., 1994, Nature, 371, 774CrossRef
Breitschwerdt, D., & Schmutzler, T., 1999, A&A, 347, 650
Breitschwerdt, D., Dogiel, V.A., & Völk, H.J., 2002, A&A, 385, 216
Cappellaro, E., Evans, R., & Turatto, M., 1999, A&A, 351, 459
Dalgarno, A., & McCray, R.A., 1972, ARA&A, 10, 375CrossRef
Everett, J.E., et al., 2008, ApJ, 674, 258CrossRef
Fuchs, B., et al., 2006, MNRAS, 373, 993CrossRef
Gressel, O., et al., A&A, 486, 35
Heiles, C., 1984, ApJS, 55, 585CrossRef
Jenkins, E.B., & Meloy, D., 1974, ApJ, 193, L121CrossRef
Joung, M.K.R., & Mac Low, M.-M., 2006, ApJ, 653, 1266CrossRef
Kahn, F.D., 1981, ASSL, 91, 1
Kompaneets, A.S., 1960, Sov. Phys. Dokl., 5, 46
Korpi, M.J., et al., 1999, ApJ, 514, 99CrossRef
Kuijken, K., & Gilmore, G., 1989, MNRAS, 239, 651CrossRef
Lockman, F.J., 1984, ApJ, 283, 90CrossRef
Mac Low, M.-M., & McCray, R., 1988, ApJ, 324, 776CrossRef
McKee, C.F., & Ostriker, J.P., 1977, ApJ, 218, 148CrossRef
Pikel’ner, S.B., 1953, Izvest. Krymsk. Astrofiz., 10, 74 (Dokl. Akad. Nauk SSSR 88, 229)Google Scholar
Salpeter, E.E., 1955, ApJ, 121, 161CrossRef
Shapiro, P.R., & Field, G.B., 1976, ApJ, 205, 762CrossRef
Spitzer, L. Jr., 1956, ApJ, 124, 20CrossRef
Sutherland, R.S., & Dopita, M.A., 1993, ApJS, 88, 253CrossRef
Tomisaka, K., & Ikeuchi, S., 1986, PASJ, 38, 697
Tomisaka, K., 1990, ApJ, 361, L5CrossRef
Wada, K., & Norman, C.A., 1999, ApJ, 516, L13CrossRef
Wang, Q.D., et al., 2001, ApJ, 555, L99CrossRef
Weaver, R., et al., 1977, ApJ, 218, 377 (Erratum 1978, 220, 742)CrossRef
Williamson, F.O., et al., 1974, ApJ, 193, L133CrossRef
Wolfire, M., et al., 1995, ApJ, 453, 673CrossRef
Tüllmann, R., et al., A&A, 448, 43
Zirakshvili, V., et al., 1996, A&A, 311, 113