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| Indexado |
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| DOI | 10.1051/0004-6361/201016117 | ||||
| Año | 2011 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Conclusions. Our sample presents the smallest fraction of asymmetric Hi profiles compared with any other yet studied. The width of the associated asymmetry parameter distribution can help to distinguish the frequency and processes of self-induced HI asymmetries, and serve as a baseline for studying asymmetry rates in other environments.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Espada, Daniel | Hombre |
Inst Astrofis Andalucia IAA CSIC - España
Natl Astron Observ Japan - Japón Instituto de Astrofísica de Andalucía - CSIC - España National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón |
| 2 | Verdes-Montenegro, Lourdes | Mujer |
Inst Astrofis Andalucia IAA CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 3 | Huchtmeier, W. K. | - |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania |
| 4 | Sulentic, J. | Hombre |
Inst Astrofis Andalucia IAA CSIC - España
Instituto de Astrofísica de Andalucía - CSIC - España |
| 5 | Verley, Simon | Hombre |
UNIV GRANADA - España
Universidad de Granada - España |
| 6 | Leon, S. | - |
Atacama Large Millimeter Array - Chile
|
| 7 | Sabater, J. | Hombre |
Inst Astrofis Andalucia IAA CSIC - España
UNIV EDINBURGH - Reino Unido Instituto de Astrofísica de Andalucía - CSIC - España University of Edinburgh, Institute for Astronomy - Reino Unido |
| Fuente |
|---|
| National Science Foundation |
| Junta de Andalucía |
| European Community |
| Cornell University |
| National Aeronautics and Space Administration |
| Junta de Andalucia (Spain) |
| National Radio Astronomy Observatory |
| DGI |
| Junta de AndalucÃa |
| Sixth Framework Programme |
| Associated Universities, Inc. |
| 6th European Community Framework Programme |
| Arecibo Observatory (National Astronomy and Ionosphere Center |
| Nancay Observatory |
| Max-Planck-Institut fuer Radioastronomie |
| Agradecimiento |
|---|
| Based on observations with the 100-m telescope of the MPIfR (Max-Planck-Institut fuer Radioastronomie) at Effelsberg, GBT under NRAO (the National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.), Arecibo Observatory (National Astronomy and Ionosphere Center, which is operated by Cornell University under a cooperative agreement with the National Science Foundation) and the Nancay Observatory. |
| Based on observations with the 100-m telescope of the MPIfR (Max-Planck-Institut fuer Radioastronomie) at Effelsberg, GBT under NRAO (the National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.), Arecibo Observatory (National Astronomy and Ionosphere Center, which is operated by Cornell University under a cooperative agreement with the National Science Foundation) and the Nançay Observatory. |