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相关论文: SDSS J042348.57-041403.5AB: A Brown Dwarf Binary S…

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With the progressive release of data from numerous sky surveys, humanity has entered the era of astronomical big data. Multi-wavelength, multi-method research is playing an increasingly crucial role. Binaries account for a substantial…

太阳与恒星天体物理 · 物理学 2025-10-14 Yanhui Chen , Chaomi Duan , Baokun Sun

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…

太阳与恒星天体物理 · 物理学 2015-05-18 Ansgar Reiners , Andreas Seifahrt , Stefan Dreizler

Benchmark brown dwarfs are those objects for which fiducial constraints are available, including effective temperature, parallax, age, metallicity. We searched for new cool brown dwarfs in 186 sq.deg. of the new area covered by the data…

太阳与恒星天体物理 · 物理学 2015-05-18 B. Goldman , S. Marsat , T. Henning , C. Clemens , J. Greiner

Most directly imaged giant exoplanets are fainter than brown dwarfs with similar spectra. To explain their relative underluminosity unusually cloudy atmospheres have been proposed. However, with multiple parameters varying between any two…

地球与行星天体物理 · 物理学 2015-06-15 Daniel Apai , Jacqueline Radigan , Esther Buenzli , Adam Burrows , Iain N. Reid , Ray Jayawardhana

We present the completion of a program to cross-correlate the SDSS Data Release 1 and 2MASS Point Source Catalog in search for extremely red L and T dwarfs. The program was initiated by Metchev and collaborators, who presented the findings…

太阳与恒星天体物理 · 物理学 2015-05-27 Kerstin Geißler , Stanimir Metchev , J. Davy Kirkpatrick , G. Bruce Berriman , Dagny Looper

We present the spectroscopic orbit of LHS 1610A, a newly discovered single-lined spectroscopic binary with a trigonometric distance placing it at 9.9 pm 0.2 pc. We obtained spectra with the TRES instrument on the 1.5m Tillinghast Reflector…

We present the spectroscopic orbits of eleven nearby, mid-to-late M dwarf binary systems in a variety of configurations: two single-lined binaries (SB1s), seven double-lined binaries (SB2s), one double-lined triple (ST2), and one…

We identify SDSSJ121010.1+334722.9 as an eclipsing post-common-envelope binary, with an orbital period of P ~ 3 hrs, containing a very cool, low-mass, DAZ white dwarf and a low-mass main-sequence star of spectral type M5. A model atmosphere…

We report the discovery of a faint L6 \pm 1 companion to the previously known M9 dwarf, 2MASS J01303563-4445411, based on our near-infrared imaging and spectroscopic observations with the 3m Infrared Telescope Facility SpeX…

太阳与恒星天体物理 · 物理学 2012-02-10 Saurav Dhital , Adam J. Burgasser , Dagny L. Looper , Keivan G. Stassun

Using astrometric measurements obtained with the FORS2/VLT camera, we are searching for low-mass companions around 20 nearby ultracool dwarfs. With a single-measurement precision of 0.1 milli-arcseconds, our survey is sensitive to a wide…

太阳与恒星天体物理 · 物理学 2015-04-29 J. Sahlmann , P. F. Lazorenko , D. Segransan , E. L. Martin , M. Mayor , D. Queloz , S. Udry

We report the discovery of the ultracool dwarf binary system J1250+0455AB, a low-mass (M$_\odot$$_\mathrm{tot} <$ 0.2 M$_\odot$) system in which the components straddle the M/L dwarf boundary. The binary was resolved through near-infrared…

太阳与恒星天体物理 · 物理学 2025-08-01 Sayan Baig , R. L. Smart , Hugh R. A. Jones , E. Pinna , A. Sozzetti , Gemma Cheng , Felice Cusano , Fabio Rossi , Cedric Plantet , Guido Agapito

We report new observations of the unusually active, high proper motion L5e dwarf 2MASS J13153094-2649513. Optical spectroscopy with Magellan/MagE reveals persistent nonthermal emission, with narrow H I Balmer, Na I and K I lines all…

太阳与恒星天体物理 · 物理学 2015-05-28 Adam J. Burgasser , Breann N. Sitarski , Christopher R. Gelino , Sarah E. Logsdon , Marshall D. Perrin

We present preliminary trigonometric parallaxes and proper motions for 22 L dwarfs and 18 T dwarfs measured using the ASTROCAM infrared imager. Relative to absolute parallax corrections are made by employing 2MASS and/or SDSS photometry for…

Using SofI on the 3.5m New Technology Telescope, we have conducted an extensive near-infrared monitoring survey of an unbiased sample of 69 brown dwarfs spanning the L0 and T8 spectral range, with at least one example of each spectral type.…

太阳与恒星天体物理 · 物理学 2014-07-02 P. A. Wilson , A. Rajan , J. Patience

We report the discovery of a substellar companion to the nearby solar-type star HD 46588 (F7V, 17.9 pc, ~3 Gyr). HD 46588 B was found through a survey for common proper motion companions to nearby stars using data from the Wide-field…

星系天体物理 · 物理学 2015-05-28 N. P. Loutrel , K. L. Luhman , P. J. Lowrance , J. J. Bochanski

We present analysis of Hubble Space Telescope images of 82 nearby field late-M and L dwarfs. We resolve 13 of these systems into double M/L dwarf systems and identify an additional possible binary. Combined with previous observations of 20…

天体物理学 · 物理学 2010-01-28 J. E. Gizis , I. N. Reid , G. R. Knapp , J. Liebert , J. D. Kirkpatrick , D. W. Koerner , A. J. Burgasser

We present new radial velocity and trigonometric parallax measurements indicating that the unusually red and photometrically variable T2 dwarf 2MASS J13243553+6358281 is a member of the young (~150 Myr) AB Doradus moving group based on its…

[ABRIDGED] We report the results of a $J$ band search for cloud-related variability in the atmospheres of 62 L4-T9 dwarfs using the Du Pont 2.5-m telescope at Las Campanas Observatory and the Canada France Hawaii Telescope on Mauna Kea. We…

太阳与恒星天体物理 · 物理学 2015-06-19 Jacqueline Radigan , David Lafrenière , Ray Jayawardhana , Etienne Artigau

Among the competing evolution theories for subdwarf-B (sdB) stars is the binary evolution scenario. EC~20117-4014 (=V4640~Sgr) is a spectroscopic binary system consisting of a pulsating sdB star and a late F main-sequence companion…

太阳与恒星天体物理 · 物理学 2018-06-13 T. Otani , T. Oswalt , A. E. Lynas-Gray , D. Kilkenny , K. Koen , M. Amaral , R. Jordan

The physical properties of brown dwarf companions found to orbit nearby, solar-type stars can be benchmarked against independent measures of their mass, age, chemical composition, and other parameters, offering insights into the evolution…