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Dust-correlated cm wavelength continuum emission from translucent clouds zeta Oph and LDN 1780
| Indexado |
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| DOI | 10.1111/J.1365-2966.2011.18562.X | ||||
| Año | 2011 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
We calculated the 31-GHz emissivities in both clouds. They are similar and have intermediate values between that of cirrus clouds and dark clouds. Nevertheless, we found an indication of an inverse relationship between emissivity and column density, which further supports the VSGs origin for the cm emission since the proportion of big relative to small grains is smaller in diffuse clouds.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | VIDAL-NAVARRO, MATIAS AMBROSIO | Hombre |
UNIV MANCHESTER - Reino Unido
Universidad de Chile - Chile University of Manchester - Reino Unido The University of Manchester - Reino Unido |
| 2 | CASASSUS-MONTERO, SIMON PABLO | Hombre |
Universidad de Chile - Chile
LUTH - Francia Univ Paris 07 - Francia GEPI - Galaxies, Etoiles, Physique, Instrumentation - Francia L'Observatoire de Paris - Francia |
| 3 | Dickinson, C. | Hombre |
UNIV MANCHESTER - Reino Unido
University of Manchester - Reino Unido The University of Manchester - Reino Unido |
| 4 | Witt, Adolf N. | Hombre |
Univ Toledo - Estados Unidos
The University of Toledo - Estados Unidos |
| 5 | Castellanos, Pablo | Hombre |
Universidad de Chile - Chile
|
| 6 | Jaffe, T. R. | Mujer |
UNIV MANCHESTER - Reino Unido
University of Manchester - Reino Unido The University of Manchester - Reino Unido |
| 7 | Jaffe, T. R. | Mujer |
UNIV MANCHESTER - Reino Unido
University of Manchester - Reino Unido The University of Manchester - Reino Unido |
| 8 | CABRERA-VIVES, GUILLERMO FELIPE | Hombre |
Universidad de Chile - Chile
|
| 9 | Cleary, K. | Hombre |
CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos |
| 10 | Allison, J. R. | Hombre |
UNIV OXFORD - Reino Unido
University of Oxford - Reino Unido |
| 11 | Bond, J. R. | Hombre |
UNIV TORONTO - Canadá
Canadian Institute for Theoretical Astrophysics - Canadá L’Institut Canadien d’Astrophysique Théorique - Canadá |
| 12 | BRONFMAN-AGUILO, MIGUEL LEONARDO | Hombre |
Universidad de Chile - Chile
|
| 13 | BUSTOS-PLACENCIA, RICARDO ARTURO | Hombre |
Universidad de Chile - Chile
Universidad de Concepción - Chile |
| 14 | Jones, M. E. | Hombre |
UNIV OXFORD - Reino Unido
University of Oxford - Reino Unido |
| 15 | Paladini, R. | Mujer |
Spitzer Sci Ctr - Estados Unidos
Spitzer Science Center - Estados Unidos |
| 16 | Pearson, T. J. | Hombre |
CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos |
| 17 | Readhead, Anthony C. S. S. | Hombre |
CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos |
| 18 | Reeves, Rodrigo | Hombre |
Universidad de Concepción - Chile
|
| 19 | Sievers, Jonathan | Hombre |
UNIV TORONTO - Canadá
Canadian Institute for Theoretical Astrophysics - Canadá L’Institut Canadien d’Astrophysique Théorique - Canadá |
| 20 | Taylor, A. C. | - |
UNIV OXFORD - Reino Unido
|
| Fuente |
|---|
| FONDECYT |
| CONICYT |
| National Science Foundation |
| NSF |
| Becas Chile |
| ERC |
| STFC |
| Royal Society |
| Seventh Framework Programme |
| Marie Curie International Incoming Fellowship |
| Chilean Center for Astrophysics FONDAP |
| Strategic Alliance for the Implementation of New Technologies (SAINT) |
| NASA/ADP |
| Kavli Operating Institute |
| Directorate for Mathematical and Physical Sciences |
| Agradecimiento |
|---|
| We are most grateful to Mika Juvela who kindly shared with us the LDN 1780 ISO images. We thank an anonymous referee for a thorough reading and very useful comments. MV acknowledges the funding from Becas Chile. SC acknowledges support from a Marie Curie International Incoming Fellowship (REA-236176), from FONDECYT grant 1100221, and from the Chilean Center for Astrophysics FONDAP 15010003. CD acknowledges an STFC Advanced Fellowship and ERC grant under FP7. LB and RB acknowledge support from CONICYT project Basal PFB-06. This work has been carried out within the framework of a NASA/ADP ROSES-2009 grant, n. 09-ADP09-0059. The CBI was supported by NSF grants 9802989, 0098734 and 0206416, and a Royal Society Small Research Grant. We are particularly indebted to the engineers who maintained and operated the CBI: Cristobal Achermann, Jose Cortes, Cristobal Jara, Nolberto Oyarace, Martin Shepherd and Carlos Verdugo. This work was supported by the Strategic Alliance for the Implementation of New Technologies (SAINT - see www.astro.caltech.edu/chajnantor/saint/index.html) and we are most grateful to the SAINT partners for their strong support. We gratefully acknowledge support from the Kavli Operating Institute and thank B. Rawn and S. Rawn Jr. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA). Support for LAMBDA is provided by the NASA Office of Space Science. We used data from the Southern H-Alpha Sky Survey Atlas (SHASSA), which is supported by the National Science Foundation. |
