Multi-zone non-thermal radiative model for stellar bowshocks
<i>Context</i>. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non-thermal radio emission has been detected so far only from the bowshock of BD+43°3654, whereas the detection of non-thermal radiation from these bowshocks at high energies remains e...
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| Autores principales: | , , , |
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| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
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2018
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| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/97308 https://ri.conicet.gov.ar/11336/82398 https://www.aanda.org/articles/aa/abs/2018/09/aa33321-18/aa33321-18.html |
| Aporte de: |
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I19-R120-10915-97308 |
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| record_format |
dspace |
| institution |
Universidad Nacional de La Plata |
| institution_str |
I-19 |
| repository_str |
R-120 |
| collection |
SEDICI (UNLP) |
| language |
Inglés |
| topic |
Astronomía Física Ciencias Exactas Acceleration of particles Radiation mechanisms: non-thermal Stars: massive Stars: winds, outflows |
| spellingShingle |
Astronomía Física Ciencias Exactas Acceleration of particles Radiation mechanisms: non-thermal Stars: massive Stars: winds, outflows Palacio, Santiago del Bosch Ramon, Valentí Müller, Ana Laura Romero, Gustavo Esteban Multi-zone non-thermal radiative model for stellar bowshocks |
| topic_facet |
Astronomía Física Ciencias Exactas Acceleration of particles Radiation mechanisms: non-thermal Stars: massive Stars: winds, outflows |
| description |
<i>Context</i>. Runaway stars produce bowshocks that are usually observed at infrared (IR) wavelengths. Non-thermal radio emission has been detected so far only from the bowshock of BD+43°3654, whereas the detection of non-thermal radiation from these bowshocks at high energies remains elusive.
<i>Aims</i>. We aim at characterising in detail the radio, X-ray, and γ-ray emission from stellar bowshocks accounting for the structure of the region of interaction between the stellar wind and its environment.
<i>Methods</i>. We develop a broadband-radiative, multi-zone model for stellar bowshocks that takes into account the spatial structure of the emitting region and the observational constraints. The model predicts the evolution and the emission of the relativistic particles accelerated and streaming together with the shocked flow.
<i>Results.</i> We present broadband non-thermal spectral energy distributions for different scenarios, synthetic radio-cm synchrotron maps that reproduce the morphology of BD+43°3654, and updated predictions in X-ray and γ-ray energy ranges. We also compare the results of the multi-zone model applied in this work with those of a refined one-zone model.
<i>Conclusions.</i> A multi-zone model provides better constraints than a one-zone model on the relevant parameters, namely the magnetic field intensity and the amount of energy deposited in non-thermal particles. However, one-zone models can be improved by carefully characterising the intensity of the IR dust photon field and the escape rate of the plasma from the shocked region. Finally, comparing observed radio maps with those obtained from a multi-zone model enables constraints to be obtained on the direction of stellar motion with respect to the observer. |
| format |
Articulo Preprint |
| author |
Palacio, Santiago del Bosch Ramon, Valentí Müller, Ana Laura Romero, Gustavo Esteban |
| author_facet |
Palacio, Santiago del Bosch Ramon, Valentí Müller, Ana Laura Romero, Gustavo Esteban |
| author_sort |
Palacio, Santiago del |
| title |
Multi-zone non-thermal radiative model for stellar bowshocks |
| title_short |
Multi-zone non-thermal radiative model for stellar bowshocks |
| title_full |
Multi-zone non-thermal radiative model for stellar bowshocks |
| title_fullStr |
Multi-zone non-thermal radiative model for stellar bowshocks |
| title_full_unstemmed |
Multi-zone non-thermal radiative model for stellar bowshocks |
| title_sort |
multi-zone non-thermal radiative model for stellar bowshocks |
| publishDate |
2018 |
| url |
http://sedici.unlp.edu.ar/handle/10915/97308 https://ri.conicet.gov.ar/11336/82398 https://www.aanda.org/articles/aa/abs/2018/09/aa33321-18/aa33321-18.html |
| work_keys_str_mv |
AT palaciosantiagodel multizonenonthermalradiativemodelforstellarbowshocks AT boschramonvalenti multizonenonthermalradiativemodelforstellarbowshocks AT mulleranalaura multizonenonthermalradiativemodelforstellarbowshocks AT romerogustavoesteban multizonenonthermalradiativemodelforstellarbowshocks |
| bdutipo_str |
Repositorios |
| _version_ |
1764820492563251203 |