Variation in the dust emissivity index across M 33 with Herschel and Spitzer (HerM 33es)

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Table 2

Images of M 33.

Wavelength	Resolution	rms noise	Telescope

500 μm	37″	8 mJy/beam	Herschel-SPIRE¹
350 μm	25″	9.2 mJy/beam	Herschel-SPIRE¹
250 μm	18″	14.1 mJy/beam	Herschel-SPIRE¹
160 μm	11″	6.9 mJy pix^-2	Herschel-PACS²
100 μm	7″	2.6 mJy pix^-2	Herschel-PACS²
70 μm	18″	10 μJy arcsec^-2	Spitzer-MIPS³
6570 Å (Hα)	2″	0.3 cm^-6 pc	KPNO⁴
HI-21 cm	17″	50 K km s^-1	VLA⁵
CO(2 − 1)	12″	0.06 K km s^-1	IRAM-30m⁵

References.

⁽¹⁾

Kramer et al. (2010); Xilouris et al. (2012);

⁽²⁾

Kramer et al. (2010); Boquien et al. (2011);

⁽³⁾

Tabatabaei et al. (2007);

⁽⁴⁾

Hoopes & Walterbos (2000);

⁽⁵⁾

Gratier et al. (2010).

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