On the shape of the mass-function of dense clumps in the Hi-GAL fields - I. Spectral energy distribution determination and global properties of the mass-functions

L. Olmi; D. Anglés-Alcázar; D. Elia; S. Molinari; L. Montier; M. Pestalozzi; S. Pezzuto; D. Polychroni; I. Ristorcelli; J. Rodon; E. Schisano; M. D. Smith; L. Testi; M. Thompson

doi:10.1051/0004-6361/201220409

Home

All issues

Volume 551 (March 2013)

A&A, 551 (2013) A111

Full HTML

Free Access

Table 2

Number of sources selected in the two SDP fields.

Region	All	Pre-stellar	Proto-stellar

ℓ = 30°	1950	929	1021
ℓ = 59°	3402	3079	323

Notes. The original sample of sources found during the source extraction and flux estimation procedure (Sect. 3.1) has been further filtered during the SED fitting procedure (Sect. 4).

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.