Source | RA | Dec | D |
![]() |
![]() |
Class |
(J2000) | (J2000) | (pc) | (
![]() |
(K) | ||
NGC 1333 IRAS 2 | 03:28:55.2 | +31:14:35 | 250 | 12.7 | 62 | 0 |
L1551 IRS 5 | 04:31:34.1 | +18:08:05.0 | 160 | 20 | 75 | 1 |
TMR 1 | 04:39:13.7 | +25:53:21 | 140 | 3.1 | 133 | 1 |
HH 46 | 08:25:43.8 | -51:00:35.6 | 450 | 16 | 102 | 1 |
Ced 110 IRS 4 | 11:06:47.0 | -77:22:32.4 | 130 | 0.8 | 55 | 1 |
BHR 71 | 12:01:36.3 | -65:08:44 | 200 | 11 | 60 | 0 |
IRAS 12496-7650 | 12:53:17.2 | -77:07:10.6 | 250 | 24 | 326b | 1 |
RCrA IRS 7Ac | 19:01:55.2 | -36:57:21.0 | 170 | - | - | 0 |
Sett.a | Ref. Cont. | Ref. CO | ||||
NGC 1333 IRAS 2 | A | 1, 2, 3, 4, 5, 6, 7 | vii | |||
L1551 IRS 5 | A | 2, 8, 9, 10, 11, 12 | i | |||
TMR 1 | AB | 13, 14, 15, 16 | i | |||
HH 46 | ABC | 1, 17, 18 | ii, iii | |||
Ced 110 IRS 4 | AB | 7,19,20,21,22 | iii, iv | |||
BHR 71 | AB | 17, 23, 24, 25 | v | |||
IRAS 12496-7650 | AB | 26, this work | iii, viii | |||
RCrA IRS 7Ac | A | 1, 7, 27, 28 | iii, viii |
a
Observed settings with CHAMP+. See Table 1.
b IRAS 12496-7650 is
likely to be viewed face-on and thus has strong IR emission and a high
.
See van Kempen et al. (2009, submitted).
c RCrA IRS 7 is a binary.
Pointing was chosen to be on RCrA IRS 7A, believed to be the main
embedded source, following results from van Kempen
et al. (2009, submitted) and Groppi
et al. (2007). RCrA IRS 7B is located 15
to the east. At mid- and
far-IR wavelengths, the source is heavily
confused with RCrA. Therefore, no reliable
and
could be derived.
Continuum References: 1: Di
Francesco et al. (2008) 2: Motte
& André (2001) 3: Gutermuth
et al. (2008)
4: Enoch et al. (2006)
5: Hatchell et al. (2007)
6: Sandell & Knee (2001)
7: Froebrich (2005)
8: Chandler & Richer (2000)
9: Reipurth et al. (2002)
10: Osorio et al. (2003)
11: Liu et al. (1996)
12: Butner et al. (1991)
13: Kenyon et al. (1994)
14: Hogerheijde et al.
(1999)
15: Furlan et al. (2008)
16: Terebey et al. (1993)
17: Henning & Launhardt
(1998)
18: van Kempen et al.
(2009)
19: Reipurth et al. (1993)
20: Luhman et al. (2008)
21: Lehtinen et al. (2001)
22: Lehtinen et al. (2003)
23: Evans et al. (2007)
24: Bourke et al. (1997)
25: Bourke (2001)
26: Henning et al. (1993)
27: Nutter et al. (2005)
28: Groppi et al. (2007)
CO references: i: Hogerheijde
et al. (1998),
ii: van Kempen et al. (2009, submitted),
iii: Paper I,
iv: Hiramatsu et al.
(2007), v: Parise
et al. (2006),
vi: Knee & Sandell (2000),
vii: Giannini et al. (2001),
viii: Giannini et al.
(1999).
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