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Infrared Parallaxes for Methane T Dwarfs
We report final results from our 2.5 yr infrared parallax program carried out with the European Southern Observatory 3.5 m New Technology Telescope and the SOFI infrared camera. Our program targetedExpand
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M dwarf spectra from 0.6 to 1.5 micron - A spectral sequence, model atmosphere fitting, and the temperature scale
Red/infrared (0.6-1.5 micron) spectra are presented for a sequence of well-studied M dwarfs ranging from M2 through M9. A variety of temperature-sensitive features useful for spectral classificationExpand
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Storm Reflectivity and Mesocyclone Evolution Associated with the 15 April 1994 Squall Line over Kentucky and Southern Indiana
Abstract A long-lived highly organized squall line moved rapidly across the middle Mississippi and Ohio Valleys on 15 April 1994 within a moderately unstable, strongly sheared environment. OverExpand
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Atypical takotsubo cardiomyopathy: dobutamine-precipitated apical ballooning with left ventricular outflow tract obstruction.
Takotsubo cardiomyopathy, or transient apical ballooning syndrome, is a recently recognized form of transient left ventricular dysfunction that is presumably caused by stress. TakotsuboExpand
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It's The Queen Calling: Phoning in HIPAA
The search for red AGN with 2MASS
We present the results of a simple, highly efficient 2MASS color-based survey that has already discovered 140 previously unknown red AGN and QSOs. These objects are near-infrared-bright andExpand
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The Classification of L Dwarfs
To highlight the need for new spectral types, a brief review of the discovery of very low luminosity dwarfs — cooler than type M9.5 — is presented. The reasoning behind the choice of letters “L” andExpand
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THE EFFECT OF BODY MASS INDEX ON HOSPITALIZATION IN HEART FAILURE WITH PRESERVED EJECTION FRACTION AND DIABETES MELLITUS
Heart failure with preserved ejection fraction (HFpEF) is a heterogeneous disorder with multi-organ involvement. The role of obesity in the pathophysiology of type 2 diabetes mellitus (DM2) and HFpEFExpand
Spectroscopic and photometric studies of main sequence M stars and a search for late-type dwarfs in the solar vicinity.
As any introductory astronomy student knows, M dwarfs are the most common stars in the Galaxy and are the faintest of the core hydrogen burners. A comprehensive study of these faint objects isExpand