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Carbon Planet Model with SiC Mantle Compound

Astronomy and Astrophysics – Astrophysics
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Carbon radio recombination line broadening effects interpretation

Astronomy and Astrophysics – Astrophysics
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Carbon radio recombination line observations of W3

Astronomy and Astrophysics – Astrophysics
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Carbon Recombination Lines and Interstellar Hydrogen Clouds.

Astronomy and Astrophysics – Astrophysics
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Carbon recombination lines and the neutral hydrogen clouds near the Orion Nebula

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Carbon recombination lines as a diagnostic of photodissociation regions

Astronomy and Astrophysics – Astrophysics
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Carbon Recombination Lines from the Galactic Plane at 34.5 & 328 MHz

Astronomy and Astrophysics – Astrophysics
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Carbon recombination lines in the Orion Bar

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Carbon Recombination Lines near 327 MHz I: "Diffuse" CII regions in the Galactic Disk

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Carbon recombination lines near 327 MHz. I. ``Diffuse'' C II regions in the Galactic Disk

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Carbon Recombination Lines toward the Riegel-Crutcher Cloud and other Cold HI Regions in the inner Galaxy

Astronomy and Astrophysics – Astrophysics – Galaxy Astrophysics
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Carbon Rich Extremely Metal Poor Stars: Signatures of Population-III AGB stars in Binary Systems

Astronomy and Astrophysics – Astrophysics
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Carbon shell flash in a 9-solar-mass star

Astronomy and Astrophysics – Astrophysics
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Carbon Star Dust from Meteorites

Astronomy and Astrophysics – Astrophysics
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Carbon star formation and neutron-rich isotope formation in low-mass asymptotic giant branch stars

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Carbon star photometry: CO and 3.2 micron bands.

Astronomy and Astrophysics – Astrophysics
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Carbon star populations in systems with different metallicities: statistics in Local Group galaxies

Astronomy and Astrophysics – Astrophysics
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Carbon star radial velocities and dark matter in the universe

Astronomy and Astrophysics – Astrophysics
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Carbon star survey in the Local Group. VII. NGC 3109 a galaxy without a stellar halo

Astronomy and Astrophysics – Astrophysics
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Carbon star survey in the Local Group. VIII. Probing the stellar halo of NGC 147

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