The 2008 outburst in the young stellar system Z CMa - I. Evidence of an enhanced bipolar wind on the AU-scale

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Table 1:

Log of the observations. R is the spectral resolution.
Date	Baseline	Projected	Position	R
		length (m)	angle ( $^\circ$ )
05/12/08	D0-G1	69	137	1500	FUOr+HBe
07/12/08	K0-G1	89	28	12 000	FUOr+HBe
09/12/08	K0-G1	88	24	12 000	FUOr+HBe
15/12/08	U2-U3	44	35	1500
	U3-U4	62	107
	U2-U4	86	78
16/12/08	U1-U2	56	35	1500
	U2-U4	77	88
	U1-U4	120	66
10/01/10	D0-G1	71	133	1500	FUOr+HBe

Notes. ``FUOr+HBe'' specifies when the binary is in the field of view.

Source LaTeX | All tables | In the text

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