EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 587 (March 2016) A&A, 587 (2016) A118 Full HTML
Highlight
Free Access

Table A.1

Dense core coordinates and dataset numbers.

Core α J2000 δ J2000 N2H+(1–0) N2D+(1–0) N2D+(2–1) C17O(1–0) Starless (s)/
(°′′′) Dataset protostellar (p)a
A3-MM1 16:26:09.7 −24:23:06 188-97 066-04 066-04 188-97 s
A-MM4 16:26:24.1 −24:21:52 188-97 066-04 066-04 188-97 s
A-MM5 16:26:25.9 −24:22:27 188-97 066-04 066-04 188-97 s
VLA1623 16:26:26.5 −24:24:31 188-97 066-04 066-04 188-97 p
SM1N 16:26:27.3 −24:23:28 188-97 066-04 066-04 188-97 s
SM1 16:26:27.5 −24:23:56 188-97 066-04 066-04 188-97 s
A-MM6 16:26:27.9 −24:22:53 188-97 066-04 066-04 188-97 s
SM2 16:26:29.5 −24:24:27 066-04 066-04 066-04 188-97 s
A-MM8 16:26:33.4 −24:25:01 066-04 066-04 066-04 – s
A-S 16:26:43.1 −24:25:42 188-97 066-04 066-04 – s
B1-MM1 16:27:08.7 −24:27:50 051-00 066-04 066-04 066-04 s
B1-MM3 16:27:12.4 −24:29:58 188-97 066-04 066-04 066-04 s
B1-MM4 16:27:15.7 −24:30:42 188-97 066-04 066-04 188-97 p?
B1B2-MM1 16:27:11.3 −24:27:39 051-00 066-04 066-04 066-04 s
B1B2-MM2 16:27:18.0 −24:28:48 051-00 066-04 – 066-04 p?
B2-MM1 16:27:17.0 −24:27:32 051-00 066-04 066-04 066-04 s
B2-MM2 16:27:20.3 −24:27:08 051-00 066-04 066-04 066-04 s
B2-MM6 16:27:25.3 −24:27:00 188-97 066-04 066-04 066-04 s
B2-MM8 16:27:28.0 −24:27:07 066-04 066-04 066-04 188-97 p?
B2-MM10 16:27:29.6 −24:27:42 188-97 066-04 066-04 066-04 p?
B2-MM14 16:27:32.8 −24:26:29 051-00 066-04 066-04 051-00 s
B2-MM15 16:27:32.8 −24:27:03 051-00 066-04 066-04 066-04 s
B2-MM16 16:27:34.5 −24:26:12 188-97 066-04 066-04 051-00 s
B2-MM17 16:27:35.2 −24:26:21 051-00 – – 051-00 s
C-We 16:26:50.0 −24:32:49 051-00 066-04 066-04 066-04 s
C-Ne 16:26:57.2 −24:31:39 051-00 066-04 066-04 051-00 s
C-MM3 16:26:58.9 −24:34:22 051-00 – – 051-00 s
C-MM4 16:26:59.4 −24:34:02 051-00 – – 051-00 s
C-MM5 16:27:00.1 −24:34:27 188-97 066-04 066-04 051-00 s
C-MM6 16:27:01.6 −24:34:37 051-00 – – 051-00 s
C-MM7 16:27:03.3 −24:34:22 051-00 – – 051-00 s
E-MM1e 16:26:57.7 −24:36:56 051-00 066-04 066-04 – s
E-MM2d 16:27:04.9 −24:39:15 188-97 066-04 066-04 051-00 s
E-MM3 16:27:05.8 −24:37:09 – – – 188-97 p
E-MM4 16:27:10.6 −24:39:30 066-04 066-04 066-04 051-00 s
E-MM5 16:27:11.8 −24:37:57 – – – 188-97 s
F-MM1 16:27:22.1 −24:40:02 066-04 066-04 066-04 188-97 s
F-MM2 16:27:24.3 −24:40:35 188-97 066-04 066-04 188-97 s
H-MM1 16:27:58.3 −24:33:42 066-04 066-04 066-04 066-04 s
I-MM1 16:28:57.7 −24:20:48 066-04 066-04 066-04 066-04 s

Notes. Given coordinates are the observed positions, the centres of the cores determined by Motte et al. (1998).

(a)

In this paper, cores are considered protostellar if they host an YSO (VLA1623, E-MM3) or if the YSO is within a half beam from the millimetre dust peak coordinates of Motte et al. (1998) used for our N2D+(1–0) survey. We label the latter cores with “p?” to indicate that the YSO is not coincident with the dust peak, so that it may have not formed within the core but it is sufficiently close to affect the core physical and chemical properties.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.