Evolution of interstellar dust and stardust in the solar neighbourhood

2007/06/08 by Svitlana Zhukovska, H. P. Gail, Hans-Peter Gail +2 · 8 citations
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Cosmic dust #Galaxy #Intergalactic dust #Interplanetary dust cloud #Interstellar cloud #Interstellar medium #Milky Way #Molecular cloud #Neighbourhood (mathematics) #Physics #Solar System #Stars #Stellar, planetary, and galactic studies #astro-ph

paper · pdf · doi:10.1051/0004-6361:20077789

29 pages, 19 figures

arxiv created 2007/06/08 · openalex publication_date 2007/12/04 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

Aims.We studied the evolution of the abundance in interstellar dust species that originate in stellar sources and from condensation in molecular clouds in the local interstellar medium of the Milky Way. We determined from this the input of dust material to the Solar System.

Citations

• α-, r-, and s-process element trends in the Galactic thin and thick disks
• The size distribution of interstellar grains
• The X‐Ray Halo of GX 5‐1
• The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems
• The Homogeneity of Interstellar Elemental Abundances in the Galactic Disk
• Elemental abundance survey of the Galactic thick disc
• Dust yields in clumpy supernova shells: SN 1987A revisited
• Nucleosynthesis yields of core-collapse supernovae and hypernovae, and galactic chemical evolution
• Dust formation in very massive primordial supernovae
• The Evolution and Explosion of Massive Stars. II. Explosive Hydrodynamics and Nucleosynthesis
• The Global Evolution of Giant Molecular Clouds. I. Model Formulation and Quasi‐Equilibrium Behavior
• The shape and composition of interstellar silicate grains
• Stellar Chemical Signatures and Hierarchical Galaxy Formation
• The evolution of the Milky Way fromits earliest phases: Constraints on stellar nucleosynthesis
• Basic physical parameters of a selected sample of evolved stars
• The Galactic supernova rate
• Isochrone ages for field dwarfs: method and application to the age–metallicity relation
• The evolution of the C/O ratio in metal-poor halo stars
• A multi-phase chemo-dynamical SPH code for galaxy evolution. Testing the code
• The WSRT wide-field H I survey

Cited by

• CAN THE GROWTH OF DUST GRAINS IN LOW-METALLICITY STAR-FORMING CLOUDS AFFECT THE FORMATION OF METAL-POOR LOW-MASS STARS?
• Effects of grain size distribution on the interstellar dust mass growth
• Nuclear astrophysics: the unfinished quest for the origin of the elements
• Dust evolution with active galactic nucleus feedback in elliptical galaxies
• SHAPING THE DUST MASS-STAR-FORMATION RATE RELATION
• Dust processing in elliptical galaxies
• CRYSTALLINE SILICATES IN EVOLVED STARS. I.SPITZER/INFRARED SPECTROGRAPH SPECTROSCOPY OF IRAS 16456–3542, 18354–0638, AND 23239+5754
• Gas-to-dust mass ratios in local galaxies over a 2 dex metallicity range