Disks and outflows in CO rovibrational emission from embedded, low-mass young stellar objects

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Table 1

Evidence for envelopes within our sample.

Source	mm-int.^a	Compact^b	Outflow^c	Ref.^d

TMC 1A	Y	Y	Y	1, 2, 3, 7
GSS 30	Y	Y	n	1, 2, 4
WL 12	Y	Y	s	1, 2, 4
Elias 29	Y	Y	Y	1, 2, 4, 8
IRS 43 S+N	Y	Y	s	1, 2, 4
IRS 44 E+W	–	Y	Y	1, 4
IRS 63	Y	Y	Y	1, 2, 4
L1551 IRS 5 AB^e	Y	Y	Y	3, 7, 13
HH 100 IRS	–	Y	Y	5, 9
WL 6	–	Y	n	1, 4
Elias 32	–	Y	–	4
CrA IRS 2	–	–	–	–
HL Tau	Y	Y	Y	3, 10, 12
SVS 20 S+N	–	Y	–	7
RNO 91	–	Y	Y	6, 11

Notes.

^(a)

Envelope detected in mm-interferometry.

^(b)

Presence of cold, compact gas centered at object position.

^(c)

Refers to cold molecular outflows detected in the (sub)-mm. (s): Molecular outflow is detected in only a single lobe. (n): No molecular outflow detected.

^(d)

The references are examples of each phenonemon and are not intended to be complete.

^(e)

Unresolved and hereafter referred to as L1551 IRS 5.

References. 1: Bontemps et al. (1996); 2: Jørgensen et al. (2009); 3: Saito et al. (2001); 4: van Kempen et al. (2009a); 5: van Kempen et al. (2009c); 6: Arce et al. (2006); 7: Gregersen et al. (2000); 8: Lommen et al. (2008); 9: Groppi et al. (2007); 10: Wilner et al. (1996); 11: Chen et al. (2009); 12: Cabrit et al. (1996); 13: Wu et al. (2009).

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