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Structural analysis of molecular cloud maps: the case of the star forming Vela-D cloud

Published online by Cambridge University Press:  01 August 2006

Davide Elia ,
F. Strafella ,
F. Massi ,
M. De Luca ,
L. Campeggio  and
B. M. T. Maiolo
Davide Elia
Affiliation:
Dipartimento di Fisica, Università di Lecce, CP 193, I-73100 Lecce, Italy email: [email protected]
F. Strafella
Affiliation:
Dipartimento di Fisica, Università di Lecce, CP 193, I-73100 Lecce, Italy email: [email protected]
F. Massi
Affiliation:
INAF – Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
M. De Luca
Affiliation:
Dipartimento di Fisica, Università degli Studi di Roma “Tor Vergata”, Via della Ricerca Scientifica 1, I-00133 Roma, Italy INAF – Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio Catone, Italy
L. Campeggio
Affiliation:
Dipartimento di Fisica, Università di Lecce, CP 193, I-73100 Lecce, Italy email: [email protected]
B. M. T. Maiolo
Affiliation:
Dipartimento di Fisica, Università di Lecce, CP 193, I-73100 Lecce, Italy email: [email protected]
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Abstract

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We present the preliminary results of a statistical analysis carried out on a 1° × 1° CO(1-0) map of the intermediate mass star forming region Vela-D Cloud. Our goal is to determine statistical parameters suitable to quantify the structure of the observed cloud, in particular the power-law exponent of the map power spectrum. Furthermore, to help in removing the degeneracy implied in using a single parameter, we also resort to the multifractal approach.

Keywords

turbulenceISM: cloudsstructurestars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 411
Copyright
Copyright © International Astronomical Union 2007

References

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