Cores, filaments, and bundles: hierarchical core formation in the L1495/B213 Taurus region

Free Access

Table 2

Dense cores in L1495/B213.

ID	α(J2000)	δ(J2000)	I(N₂H⁺)	D^a	YSO	ON^b
	()	()	(K km s^-1)	(′′)

1	04 17 43	28 08 03	1.6	140	N	5
2	04 17 50	27 56 07	1.6	81	N	–
3	04 17 56	28 12 23	1.8	149	N	–
4	04 18 04	28 08 14	1.4	114	N	8
5	04 18 04	28 22 34	1.2	87	N	7
6	04 18 06	28 05 41	2.1	157	N	8
7	04 18 10	27 35 29	1.8	135	N	9
8	04 18 34	28 27 37	2.8	177	Y^c	11
9	04 18 41	28 23 22	1.2	178	N	–
10	04 19 37	27 15 48	2.1	139	N	13a
11	04 19 44	27 13 36	2.8	123	Y^d	13b
12	04 19 52	27 11 42	1.9	100	N	–
13	04 19 59	27 10 30	2.0	116	Y^e	14
14	04 20 15	27 05 59	1.1	171	N	–
15	04 20 59	27 02 29	1.8	258	Y^f	16b
16	04 21 21	27 00 09	2.6	156	N	–
17	04 27 54	26 17 50	2.6	137	N	26b
18	04 28 02	26 19 32	1.2	99	Y^g	26b
19	04 28 14	26 20 34	2.1	134	N	–

Notes.

^(a)

FWHM of the N₂H⁺ emission (uncorrected for 60′′ beam);

^(b)

core number in the catalog of Onishi et al. (2002);

^(c)

I04152+2820;

^(d)

(4) I04166+2706;

^(e)

I04169+2702;

^(f)

2MJ04210795;

^(g)

I04248+ 2612.

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.