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Comparison of the Diffuse Halpha and FUV Continuum Backgrounds: On the Origins of the Diffuse Halpha Background
Kwang-Il Seon, Adolf Witt, Il-Joong Kim +4
We compare the diffuse H map of our Galaxy with the FUV (1370-1710Å) continuum map. The H intensity correlates well with the FUV intensity. The H/FUV intensity ratio incre…
Implications of the SPEAR FUV Maps on Our Understanding of the ISM
Eric J. Korpela, Martin Sirk, Jerry Edelstein +3
The distribution of a low-density transition temperature (10^4.5 - 10^5.5 K) gas in the interstellar medium conveys the character and evolution of diffuse matter in the Galaxy. Thi…
Precise Stellar Radial Velocities of an M Dwarf with a Michelson Interferometer and a Medium-resolution Near-infrared Spectrograph
Philip S. Muirhead, Jerry Edelstein, David J. Erskine +13
Precise near-infrared radial velocimetry enables efficient detection and transit verification of low-mass extrasolar planets orbiting M dwarf hosts, which are faint for visible-wav…