S. J. Austin
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Also affiliated: Arizona State University (1992–1996)
Research Areas
Biomedical Subjects
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Biography and Research Information
OverviewAI-generated summary
S. J. Austin's research has historically explored the analysis of astrophysical phenomena, including non-LTE spectral analysis and model constraints on supernovae like SN 1993J, and the optical and ultraviolet evolution of novae such as V1974 Cygni. More recently, Austin's work has shifted to investigate the physical and dynamical evolution of meteoroid streams, focusing on the lifetime of cm-sized zodiacal dust and properties of outer solar system pebbles during planetesimal formation. The researcher has also studied late-type near-contact eclipsing binary stars, such as [HH97] FS Aur-79. Austin holds an h-index of 5, with a total of 47 publications and 240 citations. Recent publications in 2024 indicate continued activity in the field of astro and planetary science.
Metrics
- h-index: 5
- Publications: 36
- Citations: 225
Selected Publications
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Properties of outer solar system pebbles during planetesimal formation from meteor observations (2024)
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Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams (2024)
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THE CHROMOSPHERIC ACTIVITY OF [HH97] FS Aur-79: A CLOSE BINARY WITH LATE-TYPE ACTIVE (dK7e+dM3e) COMPONENTS (2011)
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Late-Type Near-Contact Eclipsing Binary [HH97] FS Aur-79 (2007)
Collaboration Network
Top Collaborators
- Late-Type Near-Contact Eclipsing Binary [HH97] FS Aur-79
- THE CHROMOSPHERIC ACTIVITY OF [HH97] FS Aur-79: A CLOSE BINARY WITH LATE-TYPE ACTIVE (dK7e+dM3e) COMPONENTS
- Late-Type Near-Contact Eclipsing Binary [HH97] FS Aur-79
- THE CHROMOSPHERIC ACTIVITY OF [HH97] FS Aur-79: A CLOSE BINARY WITH LATE-TYPE ACTIVE (dK7e+dM3e) COMPONENTS
- Late-Type Near-Contact Eclipsing Binary [HH97] FS Aur-79
- THE CHROMOSPHERIC ACTIVITY OF [HH97] FS Aur-79: A CLOSE BINARY WITH LATE-TYPE ACTIVE (dK7e+dM3e) COMPONENTS
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
- Properties of outer solar system pebbles during planetesimal formation from meteor observations
- Lifetime of cm-sized zodiacal dust from the physical and dynamical evolution of meteoroid streams
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