The youngest massive protostars in the Large Magellanic Cloud

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Volume 518 (July-August 2010)

A&A, 518 (2010) L73

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Herschel: the first science highlights

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Table 1:

*Spitzer* and *Herschel* fluxes for YSOs discussed in Sect. 5.
Source	RA^a	Dec	Fluxes in mJy														Spitzer ID (Ref.)
	(h m s)	( $^{\circ}$ ' '')	F_J	F_H	F_K	$F_{\rm 3.6~\mu m}$	$F_{\rm 4.5~\mu m}$	$F_{\rm 5.8~\mu m}$	$F_{\rm 8.0~\mu m}$	$F_{\rm MIPS~24~\mu m}$	$F_{\rm MIPS~70~\mu m}$	$F_{\rm PACS~100~\mu m}$	$F_{\rm PACS~160~\mu m}$	$F_{\rm SPIRE~250~\mu m}$	$F_{\rm SPIRE~350~\mu m}$	$F_{\rm SPIRE~500~\mu m}$	Names
YSO-1	05:13:17.69	-69:22:25.0	1.5(0.5)	1.9(0.6)	4.8(0.8)	17(2)	29(3)	120(12)	354(35)	<3400	26 000(2600)	53 000(9600)	66 000(11000)	34 000(3400)	14 000(1400)	7300(730)	051317.69-692225.0 (1,2)
YSO-2	05:13:17.99	-69:20:04.9	0.5(0.1)	0.9(0.2)	1.2(0.4)	3.2(0.7)	2.8(0.3)	<24	<68	580(96)	2100(750)	3500(850)	5000(3500)	2800(460)	1300(330)	670(340)	...
YSO-3	05:09:58.52	-68:54:35.5	<0.2	<0.5	0.8(0.1)	1.9(0.5)	2.3(0.7)	7(1)	21(2)	250(88)	1500(680)	2100(300)	1400(300)	770(110)	430(150)	<210	050958.52-685435.5 (1)
YSO-4	05:13:01.55	-69:10:34.8	<0.1	<0.1	<0.3	0.14(0.03)	0.18(0.01)	<1	<3	8(1)	310(73)	400(51)	780(160)	630(63)	310(55)	140(61)	...

Notes. ^(a) Positions are determined from the highest-resolution images available (IRAC); few-arcsecond offsets present in this early Herschel data especially at PACS100 are accounted for in the photometry.

References. (1) Gruendl & Chu (2009); (2) Seale et al. (2009).

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