Search Results - "Ould Rouis, Lou Baya"

Using 3.4 μm Variability toward White Dwarfs as a Signpost of Remnant Planetary Systems by Guidry, Joseph A., Hermes, J. J., De, Kishalay, Ould Rouis, Lou Baya, Ewing, Brison B., Kaiser, B. C.

“…Abstract Roughly 2% of white dwarfs harbor planetary debris disks detectable via infrared excesses, but only a few percent of these disks show a gaseous…”
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A Test of Spectroscopic Age Estimates of White Dwarfs Using Wide WD+WD Binaries by Heintz, Tyler M., Hermes, J. J., Tremblay, P.-E., Ould Rouis, Lou Baya, Reding, Joshua S., Kaiser, B. C., van Saders, Jennifer L.

“…Abstract White dwarf stars have been used for decades as precise and accurate age indicators. This work presents a test of the reliability of white dwarf total…”
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Using 3.4-$\mu$m Variability towards White Dwarfs as a Signpost of Remnant Planetary Systems by Guidry, Joseph A, Hermes, J. J, De, Kishalay, Rouis, Lou Baya Ould, Ewing, Brison B, Kaiser, B. C

“…Roughly 2% of white dwarfs harbor planetary debris disks detectable via infrared excesses, but only a few percent of these disks show a gaseous component,…”
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A Test of Spectroscopic Age Estimates of White Dwarfs using Wide WD+WD Binaries by Heintz, Tyler M, Hermes, J. J, Tremblay, P. -E, Rouis, Lou Baya Ould, Redding, Joshua S, Kaiser, B. C, van Saders, Jennifer L

“…White dwarf stars have been used for decades as precise and accurate age indicators. This work presents a test of the reliability of white dwarf total ages…”
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Constraints on Remnant Planetary Systems as a Function of Main-Sequence Mass with HST/COS by Rouis, Lou Baya Ould, Hermes, J. J, Gänsicke, Boris T, Sahu, Snehalata, Koester, Detlev, Tremblay, P. -E, Veras, Dimitri, Farihi, Jay, Heintz, Tyler M, Fusillo, Nicola Pietro Gentile, Redfield, Seth

“…As the descendants of stars with masses less than 8 M$_{\odot}$ on the main sequence, white dwarfs provide a unique way to constrain planetary occurrence…”
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