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| Indexado |
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| DOI | 10.1051/0004-6361/201628176 | ||||
| Año | 2016 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Conclusions. The observed polarization percentage and polarization position angle in the present work appear consistent with those expected from longer wavelength observations in the period of 1999 2005. In particular, the polarization position angle at 492 GHz expected from the previously fitted 167 degrees +/- 7 degrees intrinsic polarization position angle and (5.6 +/- 0.7) x 105 rotation measure is 155(-8)(+98)degrees, which is consistent with our new measurement of polarization position angle within 1 sigma. The polarization percentage and the polarization position angle may be varying over the period of our ALMA 12 m Array observations, which demands further investigation with future polarization observations.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Liu, Hauyu Baobabu | - |
ESO - Alemania
Acad Sinica - Taiwán Academia Sinica, Institute of Astronomy and Astrophysics - Taiwán |
| 2 | Wright, Melvin | Hombre |
UNIV CALIF BERKELEY - Estados Unidos
University of California, Berkeley - Estados Unidos |
| 3 | Zhao, Jun-Hui | Hombre |
Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos |
| 4 | Mills, Elisabeth A. C. | Mujer |
Natl Radio Astron Observ - Estados Unidos
National Radio Astronomy Observatory Socorro - Estados Unidos |
| 5 | REQUENA-TORRES, MIGUEL ANGEL | Hombre |
Space Telescope Sci Inst - Estados Unidos
STScI - Estados Unidos Space Telescope Science Institute - Estados Unidos |
| 6 | Matsushita, Satoki | - |
Acad Sinica - Taiwán
|
| 7 | Martin, Sergio | - |
ESO - Chile
Atacama Large Millimeter Array - Chile |
| 8 | Ott, J. | Hombre |
Natl Radio Astron Observ - Estados Unidos
National Radio Astronomy Observatory Socorro - Estados Unidos |
| 9 | Morriss, M. R. | Hombre |
UNIV CALIF LOS ANGELES - Estados Unidos
University of California, Los Angeles - Estados Unidos |
| 10 | Longmore, S. N. | Hombre |
Liverpool John Moores Univ - Reino Unido
Liverpool John Moores University - Reino Unido |
| 11 | Brinkerink, Christiaan D. | Hombre |
Radboud Univ Nijmegen - Países Bajos
Radboud University Nijmegen - Países Bajos Radboud Universiteit - Países Bajos |
| 12 | Falcke, Heino | Hombre |
Radboud Univ Nijmegen - Países Bajos
Radboud University Nijmegen - Países Bajos Radboud Universiteit - Países Bajos |
| Fuente |
|---|
| National Science Foundation |
| National Science Council |
| Science and Technology Facilities Council |
| ASIAA |
| National Institutes of Natural Sciences |
| National Research Council Canada |
| National Astronomical Observatory of Japan |
| AUI/NRAO |
| Agradecimiento |
|---|
| We thank our referee for the very precise and useful opinions. H.B.L. thanks ASIAA for support. H.B.L. thanks Yu-Nung Su for the help when organizing the observational proposal; and thanks Lei Huang for some basic discussion on the subject in 2004-2006. This paper makes use of the following ALMA data: ADS/JAO.ALMA 2013.1.00071.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. We thank Aaron Evans and Todd Hunter for providing information about the ALMA primary beams. We thank Shin'ichiro Asayama, Ted Huang, Hiroshi Nagai, Dirk Petry, George Moellenbrock and Charles Hull for providing clarification on the ALMA feed orientation. |
| We thank our referee for the very precise and useful opinions. H.B.L. thanks ASIAA for support. H.B.L. thanks Yu-Nung Su for the help when organizing the observational proposal; and thanks Lei Huang for some basic discussion on the subject in 2004-2006. This paper makes use of the following ALMA data: ADS/JAO.ALMA 2013.1.00071.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. We thank Aaron Evans and Todd Hunter for providing information about the ALMA primary beams. We thank Shin'ichiro Asayama, Ted Huang, Hiroshi Nagai, Dirk Petry, George Moellenbrock and Charles Hull for providing clarification on the ALMA feed orientation. |