SIMBAD references

2016A&A...587A.106Z - Astronomy and Astrophysics, volume 587A, 106-106 (2016/3-1)

Herschel-Planck dust optical depth and column density maps. II. Perseus.

ZARI E., LOMBARDI M., ALVES J., LADA C.J. and BOUY H.

Abstract (from CDS):

We present optical depth and temperature maps of the Perseus molecular cloud, obtained combining dust emission data from the Herschel and Planck satellites and 2MASS/NIR dust extinction maps. The maps have a resolution of 36 arcsec in the Herschel regions, and of 5 arcmin elsewhere. The dynamic range of the optical depth map ranges from 1x10–2mag up to 20mag in the equivalent K-band extinction. We also evaluate the ratio between the 2.2µm extinction coefficient and the 850µm opacity. The value we obtain is close to the one found in the Orion B molecular cloud. We show that the cumulative and the differential area function of the data (which is proportional to the probability distribution function of the cloud column density) follow power laws with an index of respectively ≃-2, and ≃-3. We use WISE data to improve current YSO catalogs based mostly on Spitzer data and we build an up-to-date selection of Class I/0 objects. Using this selection, we evaluate the local Schmidt law, ΣYSO∝Σgasβ, showing that β=2.4±0.6. Finally, we show that the area-extinction relation is important for determining the star-formation rate in the cloud, which is in agreement with other recent works.

Abstract Copyright:

Journal keyword(s): ISM: clouds - dust, extinction - ISM: individual objects: Perseus molecular could - methods: data analysis - ISM: structure

VizieR on-line data: <Available at CDS (J/A+A/587/A106): tablec1.dat list.dat fits/*>

Status in Simbad:  could be processed

Simbad objects: 22

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2020.01.17-20:30:51

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