We have obtained near-infrared spectra of three L dwarfs discovered by 2MASS, 1506+13 (L3), 1507-16 (L5), and 0920+35 (L6.5). From the comparison of the H and K band spectra of these L dwarfs, we have found the presence of methane absorption in 0920+35. This implies that detectable methane absorption in the H and K bands, usually considered the signature of a T dwarf, can be present in objects classified optically as late L. Methane detection in L dwarfs is consistent with the presence of a dust layer deep in the atmosphere as the unified model of Tsuji suggests
We identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained ...
We identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained ...
One of the greatest challenges in the study of directly-imaged imaged exoplanets has been the determ...
We present 0.6--2.5 $\mu$m, R \gsim 400 spectra of twenty-seven cool, low luminosity stars and subst...
We present infrared spectra of brown dwarfs with spectral types from mid-L to T. The 0.9-2.5 $\mu$m ...
We present 0.6-2.5 mum, Rgreater than or similar to400 spectra of 27 cool, low-luminosity stars and ...
We present near-infrared spectra for a sample of T dwarfs, including 11 new discoveries made using t...
We present a spectral analysis of a sample of late L dwarfs. We use our latest model atmospheres and...
Analysis of T dwarfs using model atmospheres has been hampered by the absence of reliable line lists...
We present near-infrared spectra for a sample of T dwarfs, including 11 new discoveries made using t...
We present ZJHKL'M' photometry of a sample of 58 late M, L, and T dwarfs, most of which are identifi...
We use new and published medium resolution 0.6--2.5 $\mu$m spectra of L and T dwarfs to develop a un...
We report the discovery of four field methane ( T -type) brown dwarfs using Two Micron All-Sky Surve...
Analysis of T dwarfs using model atmospheres has been hampered by the absence of reliable line lists...
We report the discovery of four field methane ( T -type) brown dwarfs using Two Micron All-Sky Surve...
We identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained ...
We identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained ...
One of the greatest challenges in the study of directly-imaged imaged exoplanets has been the determ...
We present 0.6--2.5 $\mu$m, R \gsim 400 spectra of twenty-seven cool, low luminosity stars and subst...
We present infrared spectra of brown dwarfs with spectral types from mid-L to T. The 0.9-2.5 $\mu$m ...
We present 0.6-2.5 mum, Rgreater than or similar to400 spectra of 27 cool, low-luminosity stars and ...
We present near-infrared spectra for a sample of T dwarfs, including 11 new discoveries made using t...
We present a spectral analysis of a sample of late L dwarfs. We use our latest model atmospheres and...
Analysis of T dwarfs using model atmospheres has been hampered by the absence of reliable line lists...
We present near-infrared spectra for a sample of T dwarfs, including 11 new discoveries made using t...
We present ZJHKL'M' photometry of a sample of 58 late M, L, and T dwarfs, most of which are identifi...
We use new and published medium resolution 0.6--2.5 $\mu$m spectra of L and T dwarfs to develop a un...
We report the discovery of four field methane ( T -type) brown dwarfs using Two Micron All-Sky Surve...
Analysis of T dwarfs using model atmospheres has been hampered by the absence of reliable line lists...
We report the discovery of four field methane ( T -type) brown dwarfs using Two Micron All-Sky Surve...
We identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained ...
We identify new Y- and T-type brown dwarfs from the WISE All Sky data release using images obtained ...
One of the greatest challenges in the study of directly-imaged imaged exoplanets has been the determ...