The nearby interstellar medium toward Leo - UV observations and modeling of a warm cloud within hot gas

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Table 4

Logarithms of elemental abundances and depletion values.

	Abundance Log(X/H	Depletion^c [X/H]

C	−3.48	+ 0.06
N	−4.21	−0.11
O	−3.24	−0.00
Mg	−5.48	−1.10
Al	−7.00	−1.54
Si	−5.34	−0.95
S	−5.01	−0.27
Ar	−5.37	+ 0.01
Fe	−6.06	−1.60

Notes.

^(a)

Measured column density corrected for the ion fraction.

^(b)

Derived with N(H_tot) = 2.83 × 10¹⁸cm^-2.

^(c)

Reference abundances: the protosolar values (current solar photospheric abundances +0.074 dex to correct for gravitational settling) taken from Lodders (2003). These abundances are consistent with those used by Jenkins (2009).

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