The DOI matches its Crossref record; 41 of the 41 references it cites were found in a registry or an index.
Ionizing feedback from massive stars in massive clusters - II. Disruption of bound clusters by photoionization
Open accessAbstract
We present a smoothed particle hydrodynamics parameter study of the dynamical effect of photoionization from O-type stars on star-forming clouds of a range of masses and sizes during the time window before supernovae explode. Our model clouds all have the same degree of turbulent support initially, the ratio of turbulent kinetic energy to gravitational potential energy being set to Ekin/|Epot|= 0.7. We allow the clouds to form stars and study the dynamical effects of the ionizing radiation from the massive stars or clusters born within them. We find that dense filamentary structures and accretion flows limit the quantities of gas that can be ionized, particularly in the higher density clusters. More importantly, the higher escape velocities in our more massive (106 M⊙) clouds prevent the H ii regions from sweeping up and expelling significant quantities of gas, so that the most massive clouds are largely dynamically unaffected by ionizing feedback. However, feedback has a profound effect on the lower density 104 and 105 M⊙ clouds in our study, creating vast evacuated bubbles and expelling tens of per cent of the neutral gas in the 3-Myr time-scale before the first supernovae are expected to detonate, resulting in clouds highly porous to both photons and supernova ejecta.
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Cites
Smoothed Particle Hydrodynamics
Monaghan, J. J. (1992) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.aa.30.090192.002551 · Cited by 4,957
Embedded Clusters in Molecular Clouds
Lada, C. J., & Lada, E. A. (2003) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.41.011802.094844 · Cited by 3,034
Mass, luminosity, and line width relations of Galactic molecular clouds
Solomon, P. M., Rivolo, A. R., Barrett, J., & Yahil, A. (1987) · The Astrophysical Journal · doi:10.1086/165493 · Cited by 1,611
Embedded Clusters in Molecular Clouds
Lada, C. J., & Lada, E. A. (2003) · Cited by 1,596
André, P., Men'shchikov, A., Bontemps, S., Könyves, V., Motte, F., Schneider, N., Didelon, P., Minier, V., Saraceno, P., Ward-Thompson, D., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014666 · Cited by 1,464
The neutral atomic phases of the interstellar medium
Wolfire, M. G., Hollenbach, D., McKee, C. F., Tielens, A. G. G. M., & Bakes, E. L. O. (1995) · The Astrophysical Journal · doi:10.1086/175510 · Cited by 920
Modelling accretion in protobinary systems
Bate, M. R., Bonnell, I. A., & Price, N. M. (1995) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/277.2.362 · Cited by 910
Self-citationRE-EXAMINING LARSON'S SCALING RELATIONSHIPS IN GALACTIC MOLECULAR CLOUDS
Heyer, M., Krawczyk, C., Duval, J., & Jackson, J. M. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/699/2/1092 · Cited by 658
Churchwell, E., Povich, M. S., Allen, D., Taylor, M. G., Meade, M. R., Babler, B. L., Indebetouw, R., Watson, C., Whitney, B. A., Wolfire, M. G., et al. (2006) · The Astrophysical Journal · doi:10.1086/507015 · Cited by 554
Murray, N., Quataert, E., & Thompson, T. A. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/709/1/191 · Cited by 476
Cited by
Walch, S., Girichidis, P., Naab, T., Gatto, A., Glover, S. C. O., Wünsch, R., Klessen, R. S., Clark, P. C., Peters, T., Derigs, D., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv1975 · Cited by 366
Metadata
- Authors
- Dale, J. E., Ercolano, B., & Bonnell, I. A.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2012-06-15
- Volume
- 424
- Issue
- 1
- Pages
- 377-392
- ISSN
- 0035-8711 (ISSN-L)
- OpenAlex
- W1930544584
- Cited by
- 306
- References
- 41
- FWCI
- 15.77
- Type
- journal article
- Language
- en
- Open access
- green
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- Dale, J. E., Ercolano, B., & Bonnell, I. A. (2012). Ionizing feedback from massive stars in massive clusters - II. Disruption of bound clusters by photoionization. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2012.21205.x
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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