Free Access
   

Table 1:

Outflow status of SCUBA cores.
Source RA(J2000) Dec.(J2000) $v_{\rm LSR}$ Receiver Outflow? Class eYSO Common name
(1) (2) (3) (4) (5) (6) (7) (8)
HRF1 03:33:17.9 31:09:33.4 6.4 B y 0 (000) y b1-c
HRF2 03:33:21.4 31:07:30.7 6.8 B y 0 (000) y b1-bS
HRF4 03:33:16.3 31:06:54.3 6.7 B y 0 (000) y$^{\it b}$ b1-d
HRF5 03:33:01.9 31:04:23.2 6.6 HARP n S n  
HRF7 03:33:16.5 31:07:51.3 6.6 B y I (III) y IRAS 03301+3057, B1 SMM6
HRF10 03:33:27.3 31:07:10.1 6.6 B y I (III) y B1 SMM11
HRF12 03:43:56.5 32:00:49.9 8.8 B,HARP y,y 0 (000) y$^{\it b}$ HH211
HRF13 03:43:56.9 32:03:04.8 8.6 B y 0 (000) y IC348 MMS
HRF14 03:44:43.9 32:01:32.0 9.1 B y I (III) y$^{\it b}$  
HRF15 03:43:50.8 32:03:24.2 8.8 B,HARP y,y 0 (0I0) y$^{\it b}$ IC348 SMM3
HRF16 03:44:01.0 32:01:54.8 8.8 B,HARP n,n S n$^{\it b}$  
HRF17 03:43:57.9 32:04:01.5 8.4 B y?c13 S n  
HRF18 03:44:03.0 32:02:24.3 8.6 B,HARP n,n S n  
HRF19 03:44:36.8 31:58:48.9 9.5 B,HARP n,n S n  
HRF20 03:44:05.5 32:01:56.7 8.5 B,HARP n,n S n  
HRF21 03:44:02.3 32:02:48.5 8.6 B,HARP n,n S n  
HRF23 03:43:37.8 32:03:06.2 9.0 B,HARP n S n  
HRF24 03:43:42.3 32:03:23.2 8.7 B,HARP n,n S n  
HRF25 03:44:48.5 32:00:30.8 9.2 B,HARP n,n S n  
HRF26 03:43:44.4 32:02:55.7 8.8 B n S n  
HRF27 03:25:35.9 30:45:30.0 4.4 B y 0 (000) y L1448 NW
HRF28 03:25:36.4 30:45:15.0 4.4 B y 0 (0I0) y$^{\it b}$ L1448 N A/B
HRF29 03:25:38.8 30:44:03.6 4.8 B y 0 (000) y$^{\it b}$ L1448C
HRF30 03:25:22.4 30:45:10.7 4.1 B y 0 (000) y L1448 IRS2
HRF31 03:25:25.9 30:45:02.7 4.1 B y?c30 0 (000) n  
HRF32 03:25:49.0 30:42:24.6 4.4 HARP n?c27$^{\it a}$ S n  
HRF35 03:27:39.1 30:13:00.6 5.3 B y I (II0) y L1455 FIR4
HRF36 03:27:42.9 30:12:28.5 5.8 B y 0 (0I0) y  
HRF37 03:27:48.4 30:12:08.8 5.3 B y I (III) y L1455 PP9
HRF39 03:27:38.1 30:13:57.3 5.3 B y?c35 I (I0I) y$^{\it b}$ L1455 FIR1/2
HRF40 03:27:39.9 30:12:09.8 5.4 B y?c35,36 S n  
HRF41 03:29:10.4 31:13:30.0 7.6 B y 0 (000) y,0(6) NGC1333 IRAS 4A
HRF42 03:29:12.0 31:13:10.0 7.5 B y 0 (000) y,0(8)$^{\it b}$ NGC1333 IRAS 4B
HRF43 03:29:03.2 31:15:59.0 7.9 B y I (III) y,I(29) NGC1333 SVS13
HRF44 03:28:55.3 31:14:36.4 7.7 B y 0 (0I0) y,0(21)$^{\it f}$ NGC1333 IRAS 2A
HRF45 03:29:01.4 31:20:28.6 7.6 B y I (III) y,I(27) NGC1333 ASR 114
HRF46 03:29:11.0 31:18:27.4 7.9 B y 0 (000) y,0(7) NGC1333 ASR 32/33
HRF47 03:28:59.7 31:21:34.2 7.6 B y 0 (000) y,n NGC1333 IRAS 4C
HRF48 03:29:13.6 31:13:55.0 7.6 B y?c41,42 0 (000) y,0(9)$^{\it b}$ NGC1333 SK31
HRF49 03:28:36.7 31:13:29.6 8.0 HARP y I (III) y,I(15) NGC1333 SK6
HRF50 03:29:06.5 31:15:38.6 7.9 B y?c43,51 I (II0) n,n NGC1333 HH 7-11 MMS 4
HRF51 03:29:08.8 31:15:18.1 7.6 B y?c43,50 S n,n NGC1333 SK16
HRF52 03:29:03.7 31:14:53.1 7.6 B y?c43,50 0 (0I0) y,0(5) NGC1333 HH7-11 MMS 6
HRF53 03:29:04.5 31:20:59.1 7.6 B y?c45$^{\it d}$ S n,n NGC1333 SK26
HRF54 03:29:10.7 31:21:45.3 7.6 HARP y? c56 I (III) n,n NGC1333 SK28
HRF55 03:28:40.4 31:17:51.3 7.5 HARP y? c45,LL055 0 (000) n,n $^{\it b,g}$  
HRF56 03:29:07.7 31:21:56.8 7.6 HARP y I (III) n,I(31) NGC1333 SK29
HRF57 03:29:18.2 31:25:10.8 7.5 HARP n S n,n NGC1333 SK33
HRF58 03:29:24.0 31:33:20.8 7.5 HARP y?$^{\it a}$ 0 (I00) y,0(11)$^{\it b}$  
HRF59 03:29:16.5 31:12:34.6 7.7 HARP y?c43$^{\it a}$ S n,n  
HRF60 03:28:39.4 31:18:27.1 8.4$^{\it c}$ HARP y?c45,LL066 S n,n  
HRF61 03:29:17.3 31:27:49.6 7.6 B,HARP n,n 0 (000) y,0(10)$^{\it b}$  
HRF62 03:29:07.1 31:17:23.7 7.9 B y?c46 0 (0I0) n,n NGC1333 SK18
HRF63 03:29:18.8 31:23:16.9 7.2 HARP y?cBD  $+30^\circ~549$ I (III) y,n NGC1333 SK32
HRF64 03:29:25.5 31:28:18.1 7.9 B,HARP n,n S n,n NGC1333 Per 4A3/4D
HRF65 03:29:00.4 31:12:01.5 7.9 HARP y 0 (00I) y,0(4)$^{\it b}$ NGC1333 IRAS 4B1
HRF66 03:29:05.3 31:22:11.3 7.6 HARP y?c56$^{\it a}$ S n,n NGC1333 SK30
HRF67 03:29:19.7 31:23:56.0 7.5 HARP y I (III) y,n  
HRF68 03:28:56.2 31:19:12.5 7.7 B y?c45 0 (00I) n,n$^{\it h}$  
HRF69 03:28:34.4 31:06:59.2 7.2$^{\it c}$ HARP y?c44 I (I0I) y,n  
HRF70 03:29:15.3 31:20:31.2 8.0$^{\it c}$ HARP y?c46 0 (0I0) n,n NGC1333 SK22
HRF71 03:28:38.7 31:05:57.1 7.0$^{\it c}$ HARP y?cIRAS 03256+3055 0 (000) y,0(1)$^{\it b}$ NGC1333 HH 340B
HRF72 03:29:19.1 31:11:38.1 7.5 HARP y?c43$^{\it a}$ S n,n  
HRF74 03:28:32.5 31:11:07.7 7.5$^{\it c}$ HARP y I (I0I) y,I(12)$^{\it b}$  
HRF75 03:28:42.6 31:06:10.0 7.2$^{\it c}$ HARP y 0 (000) y,n$^{\it b}$  
HRF76 03:32:17.8 30:49:46.3 6.9 B y 0 (I00) y$^{\it b}$ IRAS 03292+3039
HRF77 03:31:21.0 30:45:27.8 7.2 B,HARP y 0 (000) y$^{\it b}$ IRAS 03282+3035
HRF78 03:47:41.6 32:51:44.0 10.0 B y I (III) y B5 IRS1
HRF79 03:47:39.1 32:52:17.9 10.0 B n S n  
HRF80 03:26:37.6 30:15:24.2 5.0 HARP n,y$^{\it a}$ I (III) y$^{\it b}$ IRAS 03235+3004
HRF81 03:30:15.5 30:23:42.8 5.9 HARP n,y?$^{\it a}$ I (III) n IRAS 03271+3013
HRF82 03:33:13.1 31:19:51.0 6.9 HARP y$^{\it a}$ S y B1 SMM1
HRF83 03:32:48.9 31:09:40.1 6.0$^{\it c}$ HARP n S n  
HRF84 03:32:21.9 31:04:55.6 6.0$^{\it c}$ HARP n 0 (I00) n  
HRF85 03:28:32.5 31:00:53.0 7.5 HARP y?$^{\it a}$ S n,I(13) IRAS 03254+3050
HRF86 03:26:30.9 30:32:27.6 4.1 HARP n 0 (000) n  
HRF88 03:31:31.6 30:43:32.2 7.2$^{\it c}$ HARP y?c77 0 (I00) n  
HRF89 03:32:25.9 30:59:05.0 6.4 HARP n S n B1 SMM9
HRF90 03:45:16.5 32:04:47.1 10.0 HARP n?$^{\it a}$ S n Per 7
HRF91 03:29:23.3 31:36:08.6 7.5$^{\it c}$ HARP n S n Per 4A
HRF101 03:44:12.8 32:01:33.9 8.6 HARP y I (III) n IRAS 03410+3152
Bolo11 03:25:46.5 30:44:17.8       S n  
Bolo26 03:28:32.7 31:04:55.9 7.0 HARP y?c65,NGC1333 S n  
Bolo27 03:28:32.7 30:19:51.1       S n  
Bolo44 03:29:04.9 31:18:41.2       S n  
Bolo62 03:30:32.3 30:26:27.4 6.0$^{\it c}$ HARP n 0 (I00) n$^{\it b}$  
Bolo64 03:30:51.3 30:49:14.7 6.0$^{\it c}$ HARP n S n  
Bolo70 03:32:44.3 31:00:09.7       S n  
Bolo89 03:40:49.3 31:48:50.1       S n  
Bolo90 03:41:09.3 31:44:38.1       I (III) n IRAS 03380+3135
Bolo92 03:41:40.7 31:57:59.8       S n  
Bolo94 03:41:46.1 31:57:22.9       S n  
Bolo111 03:44:14.4 31:57:57.6       S n  
Bolo112 03:44:15.6 32:09:15.0       I (I0I) n  
Bolo113 03:44:23.9 31:59:25.2       S n$^{\it b}$  
Bolo114 03:44:23.2 32:10:10.1       S n  
Bolo121 03:47:32.7 32:50:50.2       S n  
$^{\it a}$ There are linewings which satisfy the low-level criterion - see Sect. 3.1.2. $^{\it b}$ Contains a Spitzer LLO (Dunham et al. 2008) - see Table 3. $^{\it c}$ Uncertain $v_{\rm LSR}$ due to broad and/or weak C18O line, 13CO detection only, or velocity taken from 12CO itself. $^{\it d}$ At edge of mapped area. Possible S blue lobe. $^{\it e}$ Passed linewing criterion, but line profile suggests multiple velocity components rather than an outflow. $^{\it f}$ Gutermuth et al. (2008) Class 0 source 3 lies 30'' to the southeast of HRF44. $^{\it g}$ Gutermuth et al. (2008) Class I sources 16 and 18 lie 20'' to the south and 40'' to the southeast, respectively, of HRF55. $^{\it h}$ Gutermuth et al. (2008) Class I source 23 lies 15'' to the east of HRF68.

Source LaTeX | All tables | In the text

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.