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Table 1

Infrared detections for sources of jet objects within the Carina nebula.

Jet object Jet source Spitzer Herschel 2MASS HAWK-I

HH666 J104351.5–595521 yes yes yesa a
HH900 no yes no no
HH901 no no no yes
HH902 yes no no no
HH903 J104556.4–600608 yes yes no no
HH1004 J104644.8–601021 yes yes no no
HH1005 J104644.2–601035 yes yes no
HH1006 J104632.9–600354 yes no no no
HH1007 no no no
HH1008 J104445.4–595555 yes yes yes yes
HH1009 no no no no
HH1010 J104148.7–594338 yes yes no
HH1011 no no no no
HH1012 J104438.7–593008 yes no no no
HH1013 J104419.2–592612 yes no no no
HH1014 J104545.9–594106 yes no no no
HH1015 no no yes
HH1016 no no no no
HH1017 J104441.5–593357 yes no no no
HH1018 J104452.9–594526 yes no no no
HHc-1 J104405.4–592941 yes no no no
HHc-2 J104445.4–595555 yes yes yes yes
HHc-3 J104504.6–600303 yes no no no
HHc-4 no no no no
HHc-5 J104509.4–600203 yes yes no yes
HHc-6 J104509.2–600220 yes no no no
HHc-7 J104513.0–600259 yes no no no
HHc-8 J104512.0–600310 yes no no no
HHc-9 no no no no
HHc-10 no no no no
HHc-11 no no no no
HHc-12 no no no no
HHc-13 J104400.6–595427 yes no no
HHc-14 no no no no
HHc-15 J104353.9–593245 yes no no no
EGO J104040.5–585319 yes yes no
EGO J104248.1–592529 yes yes yes
EGO J104813.4–595848 yes yes no no
G287.10-0.73 J104114.3–593239 yes yes no
G287.95-1.13 J104542.0–601732 yes yes no
G288.15-1.17 J104700.6–602535 no no no
G288.26-1.14a J104750.3–602618 yes yes no
G288.26-1.14b J104752.1–602627 yes no no
G288.26-1.14c J104750.9–602625 yes no no
G288.26-1.14d J104751.7–602624 yes no no
CGO J104325.5–591645 yes yes no
CGO J104325.7–591660 yes yes no
CGO J104450.4–593303 yes no no no
CGO J104455.7–592554 yes yes no no
CGO J104528.6–591319 yes yes yes
MHO1605 J104351.5–593911 yes no no yes
MHO1606 no no no no
MHO1607 no no no no
MHO1608 no no no no
MHO1609 no no no no
MHO1610 yes yes no no

Notes. The Herbig-Haro objects and candidates are as detected by Smith et al. (2010a), Molecular Hydrogen objects as identified by Preibisch et al. (2011b), the Extended Green Objects bearing a number beginning with G as detected by Smith et al. (2010b). Images of them can be found in the respective source publications. The remaining four EGOs and the compact green objects were detected from our Spitzer data. For HAWK-I, where neither yes nor no are indicated the source is located outside the surveyed field.

(a)

The SOFI JHK photometry for HH666 IR was taken from Smith et al. (2004).

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