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[0 iv] Line Profiles from the Core of M 16

Astronomy and Astrophysics – Astrophysics
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[12CII] and [13CII] 158 mum emission from NGC 2024: Large column densities of ionized carbon

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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[12C]/[13C] ratios from formaldehyde in the inner galactic disk

Astronomy and Astrophysics – Astrophysics
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[alpha/Fe] in the thin and the thick disk towards an automatic parametrization of stellar spectra

Astronomy and Astrophysics – Astrophysics
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[ArIII]/[OIII] and [SIII]/[OIII]: well-behaved oxygen abundance indicators for HII regions and star forming galaxies

Astronomy and Astrophysics – Astrophysics
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[C II] emission and star formation in late-type galaxies. II A model

Astronomy and Astrophysics – Astrophysics
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[CII] 158$μ$m Emission and Metallicity in PDRs

Astronomy and Astrophysics – Astrophysics
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[CII] at 158 mic as a star formation tracer in late-type galaxies

Astronomy and Astrophysics – Astrophysics
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[CII] Emission and Star Formation in Late-Type Galaxies

Astronomy and Astrophysics – Astrophysics
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[CII] emission and star formation in the spiral arms of M31

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[CII] gas in IC 342

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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[CII] line emission in BRI1335-0417 at z=4.4

Astronomy and Astrophysics – Astrophysics – Cosmology and Extragalactic Astrophysics
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[CII] observations of H$_2$ molecular layers in transition clouds

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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[CI] 492 GHz mapping toward Cas A

Astronomy and Astrophysics – Astrophysics
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[CI] and CO in the center of M 51

Astronomy and Astrophysics – Astrophysics
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[Compton GRO Cycle 7]

Astronomy and Astrophysics – Astrophysics
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[Fe II] and H2 filaments in the Supernova Remnant G11.2-0.3: Supernova Ejecta and Presupernova Circumstellar Wind

Astronomy and Astrophysics – Astrophysics
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[Fe IV] Emission in Ionized Nebulae

Astronomy and Astrophysics – Astrophysics
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[Fe IV] emission in ionized nebulae

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[Fe NI Magnetic Dipole Transition Probabilities and the Problem of the Solar Iron Abundance

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