Direct Spectrum of the Benchmark T dwarf HD 19467 B
Crepp et al
HD 19467 B is presently the only directly imaged T dwarf companion known to induce a measurable Doppler acceleration around a solar type star. We present spectroscopy measurements of this important benchmark object taken with the Project 1640 integral field unit at Palomar Observatory. Our high-contrast R~30 observations obtained simultaneously across the JH bands confirm the cold nature of the companion as reported from the discovery article and determine its spectral type for the first time. Fitting the measured spectral energy distribution to SpeX/IRTF T dwarf standards and synthetic spectra from BT-Settl atmospheric models, we find that HD 19467 B is a T5.5+/-1 dwarf with effective temperature Teff=978+20−43 K. Our observations reveal significant methane absorption affirming its substellar nature. HD 19467 B shows promise to become the first T dwarf that simultaneously reveals its mass, age, and metallicity independent from the spectrum of light that it emits.
Friday, January 9, 2015
T Class Brown Dwarf HD 19467B's Directly Observed Spectrum
Posted by Will Baird at 12:00 PM
Labels: brown dwarf, HD 19467B, SPECTROSCOPY, T Dwarf
Subscribe to: Post Comments (Atom)
Post a Comment
Note: Only a member of this blog may post a comment.