Issue |
A&A
Volume 557, September 2013
|
|
---|---|---|
Article Number | A53 | |
Number of page(s) | 20 | |
Section | Astrophysical processes | |
DOI | https://doi.org/10.1051/0004-6361/201321160 | |
Published online | 28 August 2013 |
Planck intermediate results. XII: Diffuse Galactic components in the Gould Belt system ⋆
1
APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3,
CEA/lrfu, Observatoire de Paris,
Sorbonne Paris Cité, 10 rue Alice Domon et Léonie
Duquet,
75205
Paris Cedex 13,
France
2
Aalto University Metsähovi Radio Observatory,
Metsähovintie 114, 02540
Kylmälä,
Finland
3
African Institute for Mathematical Sciences,
6-8 Melrose Road, Muizenberg,
Cape Town, South
Africa
4
Agenzia Spaziale Italiana Science Data Center, c/o ESRIN, via
Galileo Galilei, Frascati, Italy
5
Agenzia Spaziale Italiana, Viale Liegi 26,
Roma,
Italy
6
Astrophysics Group, Cavendish Laboratory, University of
Cambridge, J J Thomson
Avenue, Cambridge
CB3 0HE,
UK
7
CITA, University of Toronto, 60 St. George St., Toronto, ON
M5S 3H8,
Canada
8
CNR – ISTI, Area della Ricerca, via G. Moruzzi 1,
Pisa,
Italy
9
CNRS, IRAP, 9
Av. colonel Roche, BP
44346, 31028
Toulouse Cedex 4,
France
10
California Institute of Technology, Pasadena, California, USA
11
Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza
San Juan, 1, planta 2, 44001
Teruel,
Spain
12
Computational Cosmology Center, Lawrence Berkeley National
Laboratory, Berkeley,
California,
USA
13
Consejo Superior de Investigaciones Científicas
(CSIC), Madrid,
Spain
14
DSM/Irfu/SPP, CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
15
DTU Space, National Space Institute, Technical University of
Denmark, Elektrovej
327, 2800
Kgs. Lyngby,
Denmark
16
Département de Physique Théorique, Université de
Genève, 24 Quai E.
Ansermet, 1211
Genève 4,
Switzerland
17
Departamento de Física Fundamental, Facultad de Ciencias,
Universidad de Salamanca, 37008
Salamanca,
Spain
18
Departamento de Física, Universidad de Oviedo,
Avda. Calvo Sotelo s/n,
Oviedo,
Spain
19
Department of Astrophysics/IMAPP, Radboud University
Nijmegen, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
20
Department of Electrical Engineering and Computer Sciences,
University of California, Berkeley, California, USA
21
Department of Physics & Astronomy, University of
British Columbia, 6224 Agricultural
Road, Vancouver, British
Columbia, Canada
22
Department of Physics and Astronomy,Dana and David Dornsife
College of Letter, Arts and Sciences, University of Southern California,
Los Angeles, CA
90089,
USA
23
Department of Physics, Gustaf Hällströmin katu 2a, University of
Helsinki, Helsinki,
Finland
24
Department of Physics, University of California,
Santa Barbara, California, USA
25
Department of Physics, University of Illinois at
Urbana-Champaign, 1110 West Green
Street, Urbana,
Illinois,
USA
26
Dipartimento di Fisica e Astronomia G. Galilei, Università degli
Studi di Padova, via Marzolo
8, 35131
Padova,
Italy
27
Dipartimento di Fisica e Scienze della Terra, Università di
Ferrara, via Saragat
1, 44122
Ferrara,
Italy
28
Dipartimento di Fisica, Università La Sapienza,
P. le A. Moro 2, Roma, Italy
29
Dipartimento di Fisica, Università degli Studi di
Milano, via Celoria
16, Milano,
Italy
30
Dipartimento di Fisica, Università degli Studi di
Trieste, via A. Valerio
2, Trieste,
Italy
31
Dipartimento di Fisica, Università di Roma Tor
Vergata, via della Ricerca
Scientifica 1, Roma, Italy
32
Dipartimento di Matematica, Università di Roma Tor
Vergata, via della Ricerca
Scientifica 1, Roma, Italy
33
Discovery Center, Niels Bohr Institute,
Blegdamsvej 17, Copenhagen, Denmark
34
Dpto. Astrofísica, Universidad de La Laguna (ULL),
38206 La Laguna, Tenerife, Spain
35
European Space Agency, ESAC, Planck Science Office, Camino bajo
del Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la
Cañada, Madrid,
Spain
36
European Space Agency, ESTEC, Keplerlaan 1,
2201 AZ
Noordwijk, The
Netherlands
37
Helsinki Institute of Physics, Gustaf Hällströmin katu 2,
University of Helsinki, Helsinki, Finland
38
INAF – Osservatorio Astronomico di Padova, Vicolo
dell’Osservatorio 5, Padova, Italy
39
INAF – Osservatorio Astronomico di Roma, via di Frascati
33, Monte Porzio
Catone, Italy
40
INAF – Osservatorio Astronomico di Trieste, via G.B. Tiepolo
11, Trieste,
Italy
41
INAF Istituto di Radioastronomia, via P. Gobetti
101, 40129
Bologna,
Italy
42
INAF/IASF Bologna, via Gobetti, 101, Bologna, Italy
43
INAF/IASF Milano, via E. Bassini 15, Milano, Italy
44
INFN, Sezione di Bologna, via Irnerio 46,
40126
Bologna,
Italy
45
INFN, Sezione di Roma 1, Universit‘a di Roma
Sapienza, Piazzale Aldo Moro
2, 00185
Roma,
Italy
46
IUCAA, Post Bag 4, Ganeshkhind, Pune University
Campus, 411 007
Pune,
India
47
Imperial College London, Astrophysics group, Blackett
Laboratory, Prince Consort
Road, London,
SW7 2AZ,
UK
48
Infrared Processing and Analysis Center, California Institute of
Technology, Pasadena,
CA
91125,
USA
49
Institut Néel, CNRS, Université Joseph Fourier Grenoble
I, 25 rue des
Martyrs, Grenoble,
France
50
Institut Universitaire de France, 103 bd Saint-Michel, 75005
Paris,
France
51
Institut d’Astrophysique Spatiale, CNRS (UMR 8617) Université
Paris-Sud 11, Bâtiment
121, Orsay,
France
52
Institut d’Astrophysique de Paris, CNRS (UMR 7095),
98 bis Boulevard Arago,
75014
Paris,
France
53
Institute for Space Sciences, Bucharest-Magurale,
Romania
54
Institute of Astronomy and Astrophysics, Academia
Sinica, Taipei,
Taiwan
55
Institute of Astronomy, University of Cambridge,
Madingley Road, Cambridge
CB3 0HA,
UK
56 Institute of Theoretical Astrophysics, University of Oslo,
Blindern, Oslo, Norway
57
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, La Laguna, Tenerife, Spain
58
Instituto de Física de Cantabria (CSIC-Universidad de
Cantabria), Avda. de los Castros
s/n, Santander,
Spain
59
Jet Propulsion Laboratory, California Institute of
Technology, 4800 Oak Grove
Drive, Pasadena,
California,
USA
60
Jodrell Bank Centre for Astrophysics, Alan Turing Building, School
of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13
9PL, UK
61
Kavli Institute for Cosmology Cambridge,
Madingley Road, Cambridge, CB3 0HA, UK
62
Kavli Institute for Theoretical Physics, University of
California, Santa Barbara Kohn
Hall, Santa
Barbara, CA
93106,
USA
63
LAL, Université Paris-Sud, CNRS/IN2P3,
Orsay,
France
64
LERMA, CNRS, Observatoire de Paris, 61 Avenue de
l’Observatoire, Paris, France
65
Laboratoire AIM, IRFU/Service d’Astrophysique – CEA/DSM – CNRS –
Université Paris Diderot, Bât. 709, CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
66
Laboratoire Traitement et Communication de l’Information, CNRS
(UMR 5141) and Télécom ParisTech, 46 rue Barrault, 75634
Paris Cedex 13,
France
67
Laboratoire de Physique Subatomique et de Cosmologie,Université
Joseph Fourier Grenoble I, CNRS/IN2P3, Institut National Polytechnique de
Grenoble, 53 rue des
Martyrs, 38026
Grenoble cedex,
France
68
Laboratoire de Physique Théorique, Université Paris-Sud 11
& CNRS, Bâtiment
210, 91405
Orsay,
France
69
Lawrence Berkeley National Laboratory,
Berkeley, California, USA
70
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741
Garching,
Germany
71
MilliLab, VTT Technical Research Centre of Finland, Tietotie
3, Espoo,
Finland
72
National University of Ireland, Department of Experimental
Physics, Maynooth,
Co. Kildare,
Ireland
73
Niels Bohr Institute, Blegdamsvej 17, Copenhagen, Denmark
74
Optical Science Laboratory, University College
London, Gower
Street, London,
UK
75
SISSA, Astrophysics Sector, via Bonomea 265,
34136
Trieste,
Italy
76
School of Physics and Astronomy, Cardiff University,
Queens Buildings, The Parade,
Cardiff, CF24 3AA, UK
77
Space Sciences Laboratory, University of California,
Berkeley, California, USA
78
Special Astrophysical Observatory, Russian Academy of
Sciences, Nizhnij Arkhyz,
Zelenchukskiy region, 369167
Karachai-Cherkessian Republic,
Russia
79
Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo
Mall, Stanford,
California,
USA
80
UPMC Univ Paris 06, UMR 7095, 98bis Boulevard Arago, 75014
Paris,
France
81
Université de Toulouse, UPS-OMP, IRAP, 31028
Toulouse Cedex 4,
France
82
Universities Space Research Association, Stratospheric Observatory
for Infrared Astronomy, MS
232-11, Moffett
Field, CA
94035,
USA
83
University of Granada, Departamento de Física Teórica y del
Cosmos, Facultad de Ciencias, Granada, Spain
84
University of Miami, Knight Physics Building, 1320
Campo Sano Dr. Coral Gables,
Florida,
USA
85
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478
Warszawa,
Poland
Received:
24
January
2013
Accepted:
31
May
2013
We perform an analysis of the diffuse low-frequency Galactic components in the southern part of the Gould Belt system (130° ≤ l ≤ 230° and −50° ≤ b ≤ −10°). Strong ultra-violet flux coming from the Gould Belt super-association is responsible for bright diffuse foregrounds that we observe from our position inside the system and that can help us improve our knowledge of the Galactic emission. Free-free emission and anomalous microwave emission (AME) are the dominant components at low frequencies (ν < 40 GHz), while synchrotron emission is very smooth and faint. We separated diffuse free-free emission and AME from synchrotron emission and thermal dust emission by using Planck data, complemented by ancillary data, using the correlated component analysis (CCA) component-separation method and we compared our results with the results of cross-correlation of foreground templates with the frequency maps. We estimated the electron temperature Te from Hα and free-free emission using two methods (temperature-temperature plot and cross-correlation) and obtained Te ranging from 3100 to 5200K for an effective fraction of absorbing dust along the line of sight of 30% (fd = 0.3). We estimated the frequency spectrum of the diffuse AME and recovered a peak frequency (in flux density units) of 25.5 ± 1.5 GHz. We verified the reliability of this result with realistic simulations that include biases in the spectral model for the AME and in the free-free template. By combining physical models for vibrational and rotational dust emission and adding the constraints from the thermal dust spectrum from Planck and IRAS, we are able to present a good description of the AME frequency spectrum for plausible values of the local density and radiation field.
Key words: Galaxy: general / radio continuum: ISM / radiation mechanisms: general
Appendices are available in electronic form at http://www.aanda.org
© ESO, 2013
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.