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Home All issues Volume 518 (July-August 2010) A&A, 518 (2010) L131 Full HTML

 


 

Table 2:

Equatorial coordinates, FWHM at 100 $\mu $m, observed fluxes with 1$\sigma $ statistical errors ( $F_{\rm PACS}$), and predicted photospheric fluxes ($F_{\star }$).

Star 		Optical position PACS 100 $\mu $m position PACS 100 $\mu $m PACS 160 $\mu $m
  (J2000) (J2000) FWHM $F_{\rm PACS}$ $F_{\star }$ $F_{\rm PACS}$ $F_{\star }$
$\delta$ Pav 20:08:43.61 -66:10:55.4 20:08:43.53 -66:10:58.1 6 $\hbox{$.\!\!^{\prime\prime}$ }3 \times 6 \hbox{$.\!\!^{\prime\prime}$ }2$ $59.6 \pm 1.1$ 68.7 $21.0 \pm 1.5$ 26.9
HR 8501 22:18:15.62 -53:37:37.5 22:18:16.14 -53:37:37.1 $6 \hbox{$.\!\!^{\prime\prime}$ }3 \times 6 \hbox{$.\!\!^{\prime\prime}$ }2$ $9.8 \pm 1.2$ 10.9   4.3
51 Peg 22:57:27.98 +20:46:07.8 22:57:28.44 +20:46:08.5 5 $\hbox{$.\!\!^{\prime\prime}$ }9 \times 6 \hbox{$.\!\!^{\prime\prime}$ }0$ $11.3 \pm 1.7$ 10.8   4.2

Notes. Absolute PACS uncertainties are $\sim$10% and less than 20% for 100 and 160 $\mu $m, respectively. Flux units are mJy.


Source LaTeX | All tables | In the text

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