The dense cores and filamentary structure of the molecular cloud in Corona Australis: Herschel SPIRE and PACS observations from the Herschel Gould Belt Survey

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Table 1

Properties of Herschel maps over all wavelengths.

Property	Wavelength (μm)

	500	350	250	160	70
HPBW (θ_beam) (′′)	36.3	24.9	18.2	13.5	8.4
Offset (MJy sr⁻¹)	4.0	9.0	16.1	19.1	2.7

Notes. The first line lists the instrumental half-power beam width (HPBW). The second line lists the offset Planck/IRAS monochromatic intensities about the CrA field (see text for details).

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