Water in star-forming regions with Herschel (WISH) - II. Evolution of 557 GHz 110–101 emission in low-mass protostars

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Volume 542 (June 2012)

A&A, 542 (2012) A8

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Table 3

Observed features in the H₂O 1₁₀–1₀₁ 557 GHz line profiles^a.

Source	Broad^b	Medium^c	Narrow^d	Bullets	Saturated abs.	Multiple abs.	Inverse P-Cygni	P-Cygni

L1448-MM	E		A	X
NGC 1333-IRAS2A	E	E	A		X
NGC 1333-IRAS4A	E	E	A+E		X		X
NGC 1333-IRAS4B	E	E	A	X^e	X
L1527	E		A+E				X
Ced110-IRS4		E	A		X
BHR71	E		A+E	X			X
IRAS 15398		E	A+E		X		X
L483		E	A		X
Ser SMM1	E	E	A		X	X
Ser SMM4	E		A+E		X	X	X
Ser SMM3	E	A	A		X	X
L723		E	A+E		X			X
B335	E		E
L1157	E		A+E	X			X

NGC 1333-IRAS3	E	A	A			X
L1489	E		A
L1551-IRS5	E		A+E		X			X
TMR1		E	A
TMC1A
TMC1	E
HH46-IRS	E		A+E					X
IRAS 12496	E		A+E		X			X
GSS30-IRS1		E	A+E		X		X
Elias 29		E	A+E		X
Oph-IRS63		E
RNO91		E
RCrA-IRS5A		E	A+E
HH100-IRS		E	E

Notes.

^(a)

Detected components marked with E (emission) or A (absorption). Detected features are marked with X.

^(b)

Δν > 20 km s^-1.

^(c)

5 < Δν < 20 km s^-1.

^(d)

Δν < 5 km s^-1.

^(e)

The bullet emission is only detected in the excited 2₀₂–1₁₁ line at 988 GHz.

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