J-Band Infrared Spectroscopy of a Sample of Brown Dwarfs Using NIRSPEC on Keck II

April 2000 • 2000ApJ...533L..45M

Authors • McLean, Ian S. • Wilcox, Mavourneen K. • Becklin, E. E. • Figer, Donald F. • Gilbert, Andrea M. • Graham, James R. • Larkin, James E. • Levenson, N. A. • Teplitz, Harry I. • Kirkpatrick, J. Davy

Abstract • Near-infrared spectroscopic observations of a sample of very cool, low-mass objects are presented with higher spectral resolution than in any previous studies. Six of the objects are L dwarfs, ranging in spectral class from L2 to L8/9, and the seventh is a methane or T dwarf. These new observations were obtained during commissioning of the near-infrared spectrometer (NIRSPEC), the first high-resolution near-infrared cryogenic spectrograph for the Keck II 10 m telescope on Mauna Kea, Hawaii. Spectra with a resolving power of R~2500 from 1.135 to 1.360 μm (approximately J band) are presented for each source. At this resolution, a rich spectral structure is revealed, much of which is due to blending of unresolved molecular transitions. Strong lines due to neutral potassium (K I) and bands due to iron hydride (FeH) and steam (H₂O) change significantly throughout the L sequence. Iron hydride disappears between L5 and L8, the steam bands deepen, and the K I lines gradually become weaker but wider because of pressure broadening. An unidentified feature occurs at 1.22 μm that has a temperature dependence like FeH but has no counterpart in the available FeH opacity data. Because these objects are 3-6 mag brighter in the near-infrared compared with the I band, spectral classification is efficient. One of the objects studied (2MASSW J1523+3014) is the coolest L dwarf discovered so far by the 2 Micron All-Sky Survey (2MASS), but its spectrum is still significantly different from the methane-dominated objects such as Gl 229B or SDSS 1624+0029. Data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.

Links

• SIMBAD http://simbad.u-strasbg.fr/simbo.pl?bibcode=2000ApJ...533L..45M
• PDF https://iopscience.iop.org/article/10.1086/312600/pdf
• PREPRINT http://arxiv.org/abs/astro-ph/0003035
• ELECTR https://doi.org/10.1086%2F312600
• SPIRES http://inspirehep.net/search?p=find+eprint+astro-ph/0003035