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相关论文: An Improbable Solution to the Underluminosity of 2…

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The properties of 2M1207b, a young (~ 8 Myr) planet-mass companion, have lacked a satisfactory explanation for some time. The combination of low luminosity, red near-IR colors, and L-type near-IR spectrum (previously consistent with Teff ~…

太阳与恒星天体物理 · 物理学 2015-05-28 Travis S. Barman , Bruce Macintosh , Quinn M. Konopacky , Christian Marois

(Abridged) Since the discovery of the first directly-imaged, planetary-mass object, 2MASS 1207 b, several works have sought to explain a disparity between its observed temperature and luminosity. Given its known age, distance, and spectral…

地球与行星天体物理 · 物理学 2016-08-14 Andrew J. Skemer , Laird M. Close , László Szűcs , Dániel Apai , Ilaria Pascucci , Beth A. Biller

In April 2004 the first image was obtained of a planetary mass companion (now known as 2M1207 b) in orbit around a self-luminous object different from our own Sun (the young brown dwarf 2MASSW J1207334-393254, hereafter 2M1207 A). 2M1207 b…

天体物理学 · 物理学 2009-11-13 C. Ducourant , R. Teixeira , G. Chauvin , G. Daigne , J. F. Le Campion , Inseok Song , B. Zuckerman

A candidate extrasolar planet companion to the young brown dwarf 2MASSW J1207334-393254 (2M1207) was recently discovered by Chauvin et al. They find that 2M1207 B's temperature and luminosity are consistent with being a young, \~5 M_Jupiter…

天体物理学 · 物理学 2009-11-13 Eric E. Mamajek

We present the first trigonometric parallax and distance for a young planetary mass object. A likely TW Hya cluster member, 2MASSW J1207334-393254Ab (hereafter 2M1207Ab) is an M8 brown dwarf with a mid to late L type planetary mass…

天体物理学 · 物理学 2009-11-13 Beth Biller , Laird Close

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…

太阳与恒星天体物理 · 物理学 2015-06-05 Jacqueline K. Faherty , Emily L. Rice , Kelle L. Cruz , Eric E. Mamajek , Alejandro Núñez

We present ALMA observations of the 2M1207 system, a young binary made of a brown dwarf with a planetary-mass companion at a projected separation of about 40 au. We detect emission from dust continuum at 0.89 mm and from the $J = 3 - 2$…

地球与行星天体物理 · 物理学 2017-07-05 L. Ricci , P. Cazzoletti , I. Czekala , S. Andrews , D. Wilner , L. Szucs , G. Lodato , L. Testi , I. Pascucci , S. Mohanty , D. Apai , J. Carpenter , B. Bowler

We report the discovery of a wide (approximately 400 AU projected separation), common proper motion companion to the nearby M dwarf LHS 2803 (PSO J207.0300-13.7422). This object was discovered during our census of the local T dwarf…

We have measured high-precision parallaxes for a large sample of candidate young (~10-100 Myr) and intermediate-age (~100-600 Myr) ultracool dwarfs, with spectral types ranging from M8 to T2.5. These objects are compelling benchmarks for…

太阳与恒星天体物理 · 物理学 2015-06-15 Michael C. Liu , Trent J. Dupuy , Katelyn N. Allers

We report the discovery of an L-type companion to the young M3.5V star 2MASS J01225093-2439505 at a projected separation of 1.45" (~52 AU) as part of our adaptive optics imaging search for extrasolar giant planets around young low-mass…

太阳与恒星天体物理 · 物理学 2015-06-16 Brendan P. Bowler , Michael C. Liu , Evgenya L. Shkolnik , Trent J. Dupuy

Upon its discovery in 2006, the young L7.5 companion to the solar analog HD 203030 was found to be unusual in being $\approx$200 K cooler than older late-L dwarfs. HD 203030B offered the first clear indication that the effective temperature…

太阳与恒星天体物理 · 物理学 2017-12-13 Paulo A. Miles-Páez , Stanimir A. Metchev , Kevin L. Luhman , Massimo Marengo , Alan Hulsebus

We have re-analyzed archival HST and Subaru data of the recently discovered planetary mass companion (PMC) GQ Lup B. With these we produce the first R and I band photometry of the companion and fit a radius and effective temperature using…

天体物理学 · 物理学 2009-11-11 C. Marois , B. Macintosh , T. Barman

Direct-imaging searches for planets reveal wide orbit planets amenable to spectroscopy, and their atmospheres represent an important comparison to the irradiated atmospheres of Hot Jupiters. Using AO integral field spectroscopy of 2M1207 b,…

地球与行星天体物理 · 物理学 2010-03-25 Jenny Patience , Robert R. King , Robert J. De Rosa , Christian Marois

We present new far-ultraviolet observations of the young M8 brown dwarf 2MASS J12073346-3932539, which is surrounded by an accretion disk. The data were obtained using the Hubble Space Telescope-Cosmic Origins Spectrograph. Moderate…

太阳与恒星天体物理 · 物理学 2015-05-18 Kevin France , Jeffrey L. Linksy , Alexander Brown , Cynthia S. Froning , Stephane Beland

We present spectroscopic analysis of the low mass binary star system GJ 660.1AB, a pair of nearby M dwarfs for which we have obtained separated near-infrared spectra (0.9-2.5 $\mu$m) with the SpeX spectrograph. The spectrum of GJ 660.1B is…

We present the discovery of a brown-dwarf companion to the 130-400 Myr-old G8 V star HD 203030. Separated by 11.9" (487 AU in projection) from its host star, HD 203030B has an estimated mass of 0.023 (+0.008;-0.011) solar masses. The K-band…

天体物理学 · 物理学 2008-11-26 Stanimir A. Metchev , Lynne A. Hillenbrand

We report the discovery of a resolved (0".9) substellar companion to a member of the 1-5 Myr Taurus star-forming region. The host star (2M0437) is a single mid-M type ($T_{eff}\approx$3100K) dwarf with a position, space motion, and…

We present a kinematic analysis of 152 low surface gravity M7-L8 dwarfs by adding 8 parallaxes, 38 radial velocities, and 19 proper motions. We find 39 objects to be high-likelihood or bona fide members of nearby moving groups, 92 objects…

We present the discovery of a candidate substellar companion from a survey of nearby, young stars with the NICMOS coronagraph on the Hubble Space Telescope. The H ~ 12 mag object was discovered approximately 4" from the young A0V star HR…

We have used multi-epoch images from the Infrared Array Camera on board the Spitzer Space Telescope to search for substellar companions to stars in the solar neighborhood based on common proper motions. Through this work, we have discovered…

星系天体物理 · 物理学 2015-05-27 K. L. Luhman , A. J. Burgasser , J. J. Bochanski
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