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Related papers: The Lowest Mass Member of the beta Pictoris Moving…

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We present new radial velocity (RV) measurements for 11 candidate young very-low-mass stars and brown dwarfs, with spectral types from M7 to L7. Candidate young objects were identified by features indicative of low surface gravity in their…

We present parallax and proper motion measurements, near-infrared spectra, and WISE photometry for the low surface gravity L5gamma dwarf 2MASSJ035523.37+113343.7 (2M0355). We use these data to evaluate photometric, spectral, and kinematic…

Solar and Stellar Astrophysics · Physics 2015-06-05 Jacqueline K. Faherty , Emily L. Rice , Kelle L. Cruz , Eric E. Mamajek , Alejandro Núñez

Substellar members of young ($\lesssim$150 Myr) moving groups are valuable benchmarks to empirically define brown dwarf evolution with age and to study the low-mass end of the initial mass function. We have combined Pan-STARRS1 (PS1) proper…

We have obtained high contrast images of four nearby, faint, and very low mass objects 2MASSJ04351455-1414468, SDSSJ044337.61+000205.1, 2MASSJ06085283-2753583 and 2MASSJ06524851-5741376 (here after 2MASS0435-14, SDSS0443+00, 2MASS0608-27…

We present first results from follow-up of targets in the northern hemisphere Beta Pictoris and AB Doradus moving group candidate list of Schlieder, Lepine, and Simon (2012). We obtained high-resolution, near-infrared spectra of 27…

Solar and Stellar Astrophysics · Physics 2015-06-11 Joshua E. Schlieder , Sebastien Lepine , Michal Simon

[Abbreviated] We present the results of a near-infrared (NIR) spectroscopic follow-up survey of 182 M4-L7 low-mass stars and brown dwarfs (BDs) from the BANYAN All-Sky Survey (BASS) for candidate members of nearby, young moving groups…

We present a new radial velocity measurement that, together with a trigonometric parallax, proper motion and signs of low gravity from the literature, confirms that SDSS J111010.01+011613.1 is a new T5.5 bona fide member of AB Doradus.…

In a recent search for unusually red L and T dwarfs, we identified 2MASS J11193254-1137466 as a likely young L7 dwarf and potential member of the TW Hydrae association. We present spectra that confirm the youth of this object. We also…

Solar and Stellar Astrophysics · Physics 2016-04-27 Kendra Kellogg , Stanimir Metchev , Jonathan Gagne , Jacqueline Faherty

Context. Though only a handful of extrasolar planets have been discovered via direct imaging, each of these discoveries had tremendous impact on our understanding of planetary formation, stellar formation and cool atmosphere physics. Aims.…

Solar and Stellar Astrophysics · Physics 2016-10-05 P. Delorme , J. Gagné , J. H. Girard , A. M. Lagrange , G. Chauvin , M-E. Naud , D. Lafrenière , R. Doyon , A. Riedel , M. Bonnefoy , L. Malo

Young brown dwarfs are analogs to giant exoplanets, as they share effective temperatures, near-infrared colors, and surface gravities. Thus, the detailed characterization of young brown dwarfs might shed light on the study of giant…

Earth and Planetary Astrophysics · Physics 2021-10-13 Elena Manjavacas , Theodora Karalidi , Johanna Vos , Beth Biller , Ben W. P. Lew

As part of our ongoing NTT SoFI survey for variability in young free-floating planets and low mass brown dwarfs, we detect significant variability in the young, free-floating planetary mass object PSO J318.5-22, likely due to rotational…

Double-lined spectroscopic binaries (SB2) allow us to determine a lower limit of the masses of their components directly to test stellar models. In this work, our aim is to derive the orbital and physical parameters of GJ1284, a young SB2.…

In a search for common proper motion companions using the VISTA Hemisphere Survey and 2MASS catalogs we have identified a very red (J-Ks=2.47 mag) late-L dwarf companion of a previously unrecognized M dwarf VHS J125601.92-125723.9, located…

Multi-band (0.9 to 1.6 um) images of the TW Hydrae Association (TWA) brown dwarf, 2MASS J1207334-393254 (also known as 2M1207), and its candidate planetary mass companion (2M1207b) were obtained on 2004 Aug 28 and 2005 Apr 26 with…

We aim at identifying very low-mass isolated planetary-mass member candidates in the nearest OB association to the Sun, Upper Scorpius (145 pc; 5-10 Myr), to constrain the form and shape of the luminosity function and mass spectrum in this…

Solar and Stellar Astrophysics · Physics 2021-03-31 N. Lodieu , N. C. Hambly , N. J. G. Cross

We describe our all-sky survey for >M4 candidate members to nearby, young associations from the 2MASS and WISE catalogs using bayesian inference. We report the first results, including 38 highly probable candidates showing spectroscopic…

Solar and Stellar Astrophysics · Physics 2013-07-05 Jonathan Gagné , David Lafrenière , René Doyon , Lison Malo , Jacqueline Faherty , Étienne Artigau

Using the Infrared Array Camera and the Multiband Imaging Photometer aboard the {\it Spitzer Space Telescope}, we have obtained images of the Lupus 3 star-forming cloud at 3.6, 4.5, 5.8, 8.0, and 24 \micron. We present photometry in these…

Astrophysics · Physics 2008-11-26 P. R. Allen , K. L. Luhman , P. C. Myers , S. T. Megeath , L. E. Allen , L. Hartmann , G. G. Fazio

Based on high-resolution spectra obtained with PHOENIX at Gemini-South, CRIRES at VLT-UT1, and ESPaDOnS at CFHT, we present new measurements of the radial and projected rotational velocities of 219 low-mass stars. The target likely…

Solar and Stellar Astrophysics · Physics 2015-06-18 Lison Malo , Étienne Artigau , René Doyon , David Lafrenière , Loïc Albert , Jonathan Gagné

Nearby young moving groups provide unique samples of similar age stars for testing the evolution of physical properties. Incomplete and/or incorrect group membership classifications reduce the usefulness of the group, which we assume to be…

Solar and Stellar Astrophysics · Physics 2019-07-17 Benjamin Kidder , Gregory Mace , Kimberly Sokal , Ricardo Lopez , Daniel Jaffe

In near-infrared NaCo observations of the young brown dwarf 2MASS J0041353-562112, we discovered a companion a little less than a magnitude fainter than the primary. The binary candidate has a separation of 143 mas, the spectral types are…

Solar and Stellar Astrophysics · Physics 2015-05-18 Ansgar Reiners , Andreas Seifahrt , Stefan Dreizler