Bipolar molecular outflow of the very low-mass star Par-Lup3-4 - Evidence for scaled-down low-mass star formation

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Table 2.

Gas properties of the ALMA detection.

Molecular	Robust	Beam size			rms	Integrated	Peak
Transition		Major axis	Minor axis	PA		Intensity ^(a)	Intensity
		[arcsec]	[arcsec]	[°]	[Jy beam⁻¹ km s⁻¹]	[Jy km s⁻¹]	[Jy beam⁻¹]
CO(3–2)	1	0.38	0.35	80	1.57 × 10⁻²	3.79	0.99
CO(2–1)	1	0.79	0.71	82	3.12 × 10⁻²	1.97	0.89
¹³CO(3–2)	2	0.41	0.37	87	4.07 × 10⁻³	8.16 × 10⁻²	5.50 × 10⁻²

Notes.

^(a)

Obtained over a 3σ contour that corresponds to an area of ∼3.8 arcsec², ∼5.0 arcsec², and ∼0.7 arcsec² for CO(3–2), CO(2–1), and ¹³CO(3–2), respectively.

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