Free Access

Table 3:

Outflow status of VeLLos and other low-luminosity embedded objects from Dunham et al. (2008).

Spitzer ID1 Submm2 Instrument Outflow? SHARC-II3 Other names/location
(1) (2) (3) (4) (5) (6) (7)
65 J032900.55+311200.7 HRF71 HARP y?cLL068 y southwest of NGC1333
73 J032912.07+311301.6 HRF42 B y - NGC1333 IRAS4B
108 J034402.64+320159.5 HRF16 HARP n n in IC348 horseshoe by 107
Low luminosity objects ( Dunham et al. 2008 groups 1-4, probably embedded)
55 J032536.22+304515.8 HRF28 B y - L1448NW
56 J032539.12+304358.1 HRF29 B y - L1448C
60 J032637.46+301528.1 HRF80 HARP y y IRAS 03235+3004
63 J032738.26+301358.8 HRF39 B y - L1455 FIR1/2
64 J032832.57+311105.3 HRF74 HARP y y  
68 J032845.29+310542.0 HRF75 HARP y y 30'' southeast of the submm peak
71 J032900.55+311200.7 HRF65 HARP y y  
74 J032913.54+311358.1 HRF48 B y?a cHRF42 - NGC1333 IRAS4C
75 J032917.16+312746.4 HRF61 HARP n y N of NGC1333
78 J032923.47+313329.5 HRF58 HARP yb y N of NGC1333
80 J032951.82+313906.1 - - - - Far north of NGC1333, outside SCUBA map.
81 J033032.69+302626.5 Bolo62 HARP y?$^{\it b}$cHRF81 y NE of IRAS03271+3013 (HRF81)
84 J033120.98+304530.2 HRF77 B y - IRAS03282+3035
88 J033217.95+304947.6 HRF76 B y - IRAS03292+3039
90 J033229.18+310240.9 - HARP y y W of B1. Weak 850  $\mu {\rm m}$ emission peaks 10'' SSW.
92 J033314.38+310710.9 HRF4 B y - NW of the submm peak
93 J033316.44+310652.6 HRF4 B y - Coincident with submm peak
104 J034351.02+320307.9 HRF15 B/HARP y y IC348-SMM3c
105 J034356.52+320052.9 HRF12 B y - HH211
106 J034356.83+320304.7 HRF14 B y - IC348 mms
107 J034402.40+320204.9 HRF16 HARP n n in IC348 horseshoe by 108
109 J034421.36+315932.6 Bolo113 - -    
Low Luminosity objects observed by HARP (groups 5-6, likely not embedded)
66 J032843.58+311736.2 HRF55 HARP y?c45 n W of NGC1333
76 J032919.75+311256.9 - HARP y?c46,LL077 n SW of NGC1333 IRAS4B
77 J032920.35+311250.4 - HARP y?c46,LL076 n SW of NGC1333 IRAS4B
a The NGC1333 IRAS4C outflow status is uncertain from the R$\times $B maps (Paper III). b Flows detected by the lower linewing criterion (Sect. 3.1.2). c There is an additional Spitzer source to the north (``LL104N'') which is not classified as a LLO but appears to be the outflow driving source.

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.