Bibcode
Planck Collaboration; Ade, P. A. R.; Aghanim, N.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Balbi, A.; Banday, A. J.; Barreiro, R. B.; Bartlett, J. G.; Battaner, E.; Benabed, K.; Benoît, A.; Bernard, J.-P.; Bersanelli, M.; Bhatia, R.; Bock, J. J.; Bonaldi, A.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Boulanger, F.; Bucher, M.; Burigana, C.; Cabella, P.; Cantalupo, C. M.; Cardoso, J.-F.; Catalano, A.; Cayón, L.; Challinor, A.; Chamballu, A.; Chary, R.-R.; Chiang, L.-Y.; Christensen, P. R.; Clements, D. L.; Colombi, S.; Couchot, F.; Coulais, A.; Crill, B. P.; Cuttaia, F.; Danese, L.; Davies, R. D.; Davis, R. J.; de Bernardis, P.; de Gasperis, G.; de Rosa, A.; de Zotti, G.; Delabrouille, J.; Delouis, J.-M.; Désert, F.-X.; Dickinson, C.; Dobashi, K.; Donzelli, S.; Doré, O.; Dörl, U.; Douspis, M.; Dupac, X.; Efstathiou, G.; Enßlin, T. A.; Falgarone, E.; Finelli, F.; Forni, O.; Frailis, M.; Franceschi, E.; Galeotta, S.; Ganga, K.; Giard, M.; Giardino, G.; Giraud-Héraud, Y.; González-Nuevo, J.; Górski, K. M.; Gratton, S.; Gregorio, A.; Gruppuso, A.; Hansen, F. K.; Harrison, D.; Helou, G.; Henrot-Versillé, S.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Hovest, W.; Hoyland, R. J.; Huffenberger, K. M.; Jaffe, A. H.; Joncas, G.; Jones, W. C.; Juvela, M.; Keihänen, E.; Keskitalo, R.; Kisner, T. S.; Kneissl, R.; Knox, L.; Kurki-Suonio, H.; Lagache, G.; Lamarre, J.-M.; Lasenby, A. et al.
Bibliographical reference
Astronomy and Astrophysics, Volume 536, id.A23
Advertised on:
12
2011
Journal
Citations
173
Refereed citations
152
Description
We present the statistical properties of the Cold Clump Catalogue of
Planck Objects (C3PO), the first all-sky catalogue of cold objects, in
terms of their spatial distribution, dust temperature, distance, mass,
and morphology. We have combined Planck and IRAS data to extract 10342
cold sources that stand out against a warmer environment. The sources
are distributed over the whole sky, including in the Galactic plane,
despite the confusion, and up to high latitudes (>30°). We find a
strong spatial correlation of these sources with ancillary data tracing
Galactic molecular structures and infrared dark clouds where the latter
have been catalogued. These cold clumps are not isolated but clustered
in groups. Dust temperature and emissivity spectral index values are
derived from their spectral energy distributions using both Planck and
IRAS data. The temperatures range from 7K to 19K, with a distribution
peaking around 13K. The data are inconsistent with a constant value of
the associated spectral index β over the whole temperature range:
β varies from 1.4 to 2.8, with a mean value around 2.1. Distances
are obtained for approximately one third of the objects. Most of the
detections lie within 2kpc of the Sun, but more distant sources are also
detected, out to 7kpc. The mass estimates inferred from dust emission
range from 0.4 M&sun; to 2.4 × 105
M&sun;. Their physical properties show that these cold
sources trace a broad range of objects, from low-mass dense cores to
giant molecular clouds, hence the "cold clump" terminology. This first
statistical analysis of the C3PO reveals at least two colder populations
of special interest with temperatures in the range 7 to 12K: cores that
mostly lie close to the Sun; and massive cold clumps located in the
inner Galaxy. We also describe the statistics of the early cold core
(ECC) sample that is a subset of the C3PO, containing only the 915 most
reliable detections. The ECC is delivered as a part of the Planck Early
Release Compact Source Catalogue (ERCSC).
Corresponding author: L. Montier, e-mail: Ludovic.Montier [at] irap.omp.eu (Ludovic[dot]Montier[at]irap[dot]omp[dot]eu)
Related projects
Anisotropy of the Cosmic Microwave Background
The general goal of this project is to determine and characterize the spatial and spectral variations in the temperature and polarisation of the Cosmic Microwave Background in angular scales from several arcminutes to several degrees. The primordial matter density fluctuations which originated the structure in the matter distribution of the present
Rafael
Rebolo López