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Name | RA, Dec (J2000) | Type | ![]() |
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100 ![]() |
160 ![]() |
250 ![]() |
350 ![]() |
500 ![]() |
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R71 | 05![]() ![]() ![]() ![]() ![]() ![]() |
LBV | ![]() |
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IRAS05280-6910 | 05![]() ![]() ![]() ![]() ![]() ![]() |
RSG, OH/IR | ... | ... | ![]() |
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<![]() |
HD 36402 | 05![]() ![]() ![]() ![]() ![]() ![]() |
WC4(+O?)+O8I | ... | ... | ... | ... | ... |
HD 36402 IR1/YSO2 | 05![]() ![]() ![]() ![]() ![]() ![]() |
YSO? | ![]() |
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<![]() |
<![]() |
Notes. Quoted
uncertainties are 1
.
Upper limits are either below the 3
detection level or include substantial flux from an adjacent unresolved
source. IRAS05280-6910 does not fall within the PACS coverage. The WR
star itself is not resolved in Herschel images; it
is severely blended with an IR source (IR1/YSO2). The 350 and
500
m
fluxes of IR1/YSO2 include a nearby YSO (N51-YSO1), which is unresolved
from IR1/YSO2 at these wavelengths. Aperture corrections for PACS and
SPIRE were
estimated using the current point-spread functions, and are
roughly 1.4 and 1.2, respectively. None of the
sources are heavily affect by high and/or variable backgrounds
(Fig. 1).



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