activity
20092023
most citedSpeX Spectroscopy of Unresolved Very Low Mass Binaries. II. Identification of Fourteen Candidate Binaries with Late-M/Early-L and T Dwarf Components

136 citations · 554 across the 15 of their papers we have counts for

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Showing 2012Show all

5 papers · 1 filter

astro-ph.SR2012

The kinematics of very low mass dwarfs: splinter session summary

Adam J. Burgasser, Jacqueline K. Faherty, Sarah Schmidt +10

Kinematic investigations are being increasingly deployed in studies of the lowest mass stars and brown dwarfs to investigate their origins, characterize their atmospheres, and exam…

astro-ph.SR2012★ 45 cited

Discovery of a Very Low Mass Triple with Late-M and T Dwarf Components: LP 704-48/SDSS J0006-0852AB

Adam J. Burgasser, Christopher Luk, Saurav Dhital +5

We report the identification of the M9 dwarf SDSS J000649.16-085246.3 as a spectral binary and radial velocity variable with components straddling the hydrogen burning mass limit.…

astro-ph.SR2012★ 63 cited

Predicting the Fate of Binary Red Giants Using the Observed Sequence E Star Population: Binary Planetary Nebula Nuclei and Post-RGB Stars

J. D. Nie, P. R. Wood, C. P. Nicholls

Sequence E variables are close binary red giants that show ellipsoidal light variations. They are likely the immediate precursors of planetary nebulae (PNe) with close binary centr…

astro-ph.SR2012

Why variable AGB stars with Long Secondary Periods aren't binaries, but are dusty

C. P. Nicholls

Roughly 30% of variable AGB stars show a Long Secondary Period, or LSP. These LSPs have posed something of a problem in recent years and their cause remains a mystery. By combining…

astro-ph.SR2012★ 28 cited

Eccentric Ellipsoidal Red Giant Binaries in the LMC: Complete Orbital Solutions and Comments on Interaction at Periastron

C. P. Nicholls, P. R. Wood

Modelling ellipsoidal variables with known distances can lead to exact determination of the masses of both components, even in the absence of eclipses. We present such modelling us…