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20032009
most citedThe Boundary Conditions of the Heliosphere: Photoionization Models Constrained by Interstellar and In Situ Data

137 citations · 173 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2009

Dust Formation in the young core-collapse supernova remnant E0102

J. Rho, W. T. Reach, A. Tappe +4

We present Spitzer IRS and IRAC observations of the young supernova remnant E0102 (SNR 1E0102.2-7219) in the Small Magellanic Cloud. The infrared spectra show strong ejecta lines o…

astro-ph.SR20093 cited

Dust Formation Observed in Young Supernova Remnants with Spitzer

J. Rho, W. T. Reach, A. Tappe +8

We present dust features and masses observed in young supernova remnants (SNRs) with Spitzer IRS mapping and staring observations of four youngest supernova remnants: SNR 1E102.2-7…

astro-ph200825 cited

The Origins and Physical Properties of the Complex of Local Interstellar Clouds

Jonathan D. Slavin

The Complex of Local Interstellar Clouds (CLIC) is a relatively tight grouping of low density, warm, partially ionized clouds within about 15 pc of the Solar System. The Local Inte…

astro-ph20078 cited

X-Atlas: An Online Archive of Chandra's Stellar High Energy Transmission Gratings Observations

Owen W. Westbrook, Nancy Remage Evans, Scott J. Wolk +6

The high-resolution X-ray spectroscopy made possible by the 1999 deployment of the Chandra X-ray Observatory has revolutionized our understanding of stellar X-ray emission. Many pu…

astro-ph2007137 cited

The Boundary Conditions of the Heliosphere: Photoionization Models Constrained by Interstellar and In Situ Data

Jonathan D. Slavin, Priscilla C. Frisch

The boundary conditions of the heliosphere are set by the ionization, density and composition of inflowing interstellar matter. Constraining the properties of the Local Interstella…

astro-ph2006

Evaporation and Thermal Balance of Tiny HI Clouds

Jonathan D. Slavin

We discuss the thermal evaporation of tiny HI clouds in the interstellar medium. Cold neutral clouds will take ~10^6 - 10^7 yr to evaporate if they are embedded in warm neutral gas…