O and O observations of ρ Ophiuchi A | Astronomy & Astrophysics (A&A)

Free Access

Table 4:

Gaussian parameters of $^{{13}}{{\rm C}}^{{18}}{{\rm O}}$ (3-2) and O₂ (1₁-1₀) lines.
Molecular	$\upsilon _{\rm LSR}$	FWHM	$T_{\rm peak}$	Note
spectral line	(km s^-1)	(km s^-1)	(K)
O₂ 119 GHz	3.5	1.5^a	$17.4\times 10^{-3}$	observed 10 $^{\prime }$ beam
${{\rm C}}^{{18}}{{\rm O}}$ 329 GHz	3.2	1.4	2.9	convolved 10 $^{\prime }$ beam
${{\rm C}}^{{18}}{{\rm O}}$ 329 GHz	3.6	1.0	16.5	observed 19 $^{\prime \prime }$ beam, P 3

Notes. ^(a) The O₂ line is artifically broadened (see Larsson et al. 2007).

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.