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相关论文: Large Scale Searches for Brown Dwarfs and Free-Flo…

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Studies of brown dwarfs as a distinct galactic population have been largely pioneered by dedicated, vast-area surveys at deep optical and near-infrared wavebands. The Two Micron All Sky Survey has, because of its full-sky coverage and…

天体物理学 · 物理学 2007-05-23 J. Davy Kirkpatrick

We report the results of a deep near infrared (JHK) survey of the outer parts of the Trapezium Cluster with Gemini South/Flamingos. 396 sources were detected in a 26 arcmin^2 area, including 138 brown dwarf candidates, defined as M<0.075…

天体物理学 · 物理学 2009-11-11 P. W. Lucas , P. F. Roche , M. Tamura

To date the search for habitable Earth-like planets has primarily focused on nuclear burning stars. I propose that this search should be expanded to cool white dwarf stars that have expended their nuclear fuel. I define the continuously…

地球与行星天体物理 · 物理学 2011-03-30 Eric Agol

Widefield surveys have always provided a rich hunting ground for the coolest stars and brown dwarfs. The single epoch surveys at the beginning of this century greatly expanded the parameter space for ultracool dwarfs. Here we outline the…

We propose to use Kepler in 2-wheel mode to conduct a detailed search for Earth-sized planets orbiting ultra-cool stars and brown dwarfs (spectral types from M7 to L3). This population of objects presents several advantages for exoplanet…

Sun-like stars have stellar, brown dwarf and planetary companions. To help constrain their formation and migration scenarios, we analyse the close companions (orbital period < 5 years) of nearby Sun-like stars. By using the same sample to…

天体物理学 · 物理学 2009-11-10 Daniel Grether , Charles H. Lineweaver

M dwarfs are favorable targets for exoplanet detection with current instrumentation, but stellar companions can induce false positives and inhibit planet characterization. Knowledge of stellar companions is also critical to our…

The discovery of extra-solar planets is one of the greatest achievements of modern astronomy. The detection of planets with a wide range of masses demonstrates that extra-solar planets of low mass exist. In this paper we describe a mission,…

The last few years has seen a dramatic increase in the number of exoplanets known and in the range of methods for characterising their atmospheric properties. At the same time, new discoveries of increasingly cooler brown dwarfs have pushed…

地球与行星天体物理 · 物理学 2015-06-23 Jeremy Bailey

Context. Thanks to recent and ongoing large scale surveys, hundreds of brown dwarfs have been discovered in the last decade. The Canada-France Brown Dwarf Survey is a wide-field survey for cool brown dwarfs conducted with the MegaCam camera…

太阳与恒星天体物理 · 物理学 2015-05-19 C. Reyle , P. Delorme , C. J. Willott , L. Albert , X. Delfosse , T. Forveille , E. Artigau , L. Malo , G. J. Hill , R. Doyon

In anticipation of the VLT/SPHERE planet imager guaranteed time programs, we have conducted a preparatory survey of 86 stars between 2009 and 2013 in order to identify new faint comoving companions to ultimately carry out a comprehensive…

Despite the recent discoveries of planets orbiting stars at all evolutionary stages, the evolution of planetary systems remains poorly understood. Studying planetary systems around red giant branch stars can reveal how main sequence…

地球与行星天体物理 · 物理学 2024-10-23 Samuel K. Grunblatt

Brown dwarfs are essential probes of stellar and planetary formation, yet their low luminosities pose challenges for detection at large Galactic distances. The James Webb Space Telescope (JWST), with its unprecedented near-infrared…

太阳与恒星天体物理 · 物理学 2025-10-03 Zhijun Tu , Shu Wang , Xiaodian Chen , Jifeng Liu

Over the past decades, direct imaging has confirmed the existence of substellar companions (exoplanets or brown dwarfs) on wide orbits (>10 au) from their host stars. To understand their formation and evolution mechanisms, we have initiated…

地球与行星天体物理 · 物理学 2021-07-14 M. Langlois , R. Gratton , A. -M. Lagrange , P. Delorme , A. Boccaletti , M. Bonnefoy , A. -L. Maire , D. Mesa , G. Chauvin , S. Desidera , A. Vigan , A. Cheetham , J. Hagelberg , M. Feldt , M. Meyer , P. Rubini , H. Le Coroller , F. Cantalloube , B. Biller , M. Bonavita , T. Bhowmik , W. Brandner , S. Daemgen , V. D'Orazi , O. Flasseur , C. Fontanive , R. Galicher , J. Girard , P. Janin-Potiron , M. Janson , M. Keppler , T. Kopytova , E. Lagadec , J. Lannier , C. Lazzoni , R. Ligi , N. Meunier , A. Perreti , C. Perrot , L. Rodet , C. Romero , D. Rouan , M. Samland , G. Salter , E. Sissa , T. Schmidt , A. Zurlo , D. Mouillet , L. Denis , E. Thiebaut , J. Milli , Z. Wahhaj , J. -L. Beuzit , C. Dominik , Th. Henning , F. Menard , A. Muller , H. M. Schmid , M. Turatto , S. Udry , L. Abe , J. Antichi , F. Allard , A. Baruffolo , P. Baudoz , J. Baudrand , A. Bazzon , P. Blanchard , M. Carbillet , M. Carle , E. Cascone , J. Charton , R. Claudi , A. Costille , V. De Caprio , A. Delboulbe , K. Dohlen , D. Fantinel , P. Feautrier , T. Fusco , P. Gigan , E. Giro , D. Gisler , L. Gluck , C. Gry , N. Hubin , E. Hugot , M. Jaquet , M. Kasper , D. Le Mignant , M. Llored , F. Madec , Y. Magnard , P. Martinez , D. Maurel , S. Messina , O. Moller-Nilsson , L. Mugnier , T. Moulin , A. Origne , A. Pavlov , D. Perret , C. Petit , J. Pragt , P. Puget , P. Rabou , J. Ramos , F. Rigal , S. Rochat , R. Roelfsema , G. Rousset , A. Roux , B. Salasnich , J. F. Sauvage , A. Sevin , C. Soenke , E. Stadler , M. Suarez , L. Weber , F. Wildi , E. Rickman

Practically all known planet hosts will evolve into white dwarfs, and large parts of their planetary systems will survive this transition - the same is true for the solar system beyond the orbit of Mars. Spectroscopy of white dwarfs…

According to various estimates, brown dwarfs (BD) should account for up to 25 percent of all objects in the Galaxy. However, few of them are discovered and well-studied, both individually and as a population. Homogeneous and complete…

太阳与恒星天体物理 · 物理学 2023-08-21 Aleksandra Avdeeva

We present design considerations for a ground-based survey for transiting exoplanets around L and T dwarfs, spectral classes that have yet to be thoroughly probed for planets. We simulate photometry for L and T targets with a variety of…

地球与行星天体物理 · 物理学 2019-10-09 Patrick Tamburo , Philip S. Muirhead

The Backyard Worlds: Planet 9 citizen science project uses data from the Wide-field Infrared Survey Explorer to detect infrared objects with significant motion. In this work, we present the majority of the L and T dwarf candidates…

The last decade of direct imaging (DI) searches for sub-stellar companions has uncovered a widely diverse sample that challenges the current formation models, while highlighting the intrinsically low occurrence rate of wide companions,…

太阳与恒星天体物理 · 物理学 2022-05-31 M. Bonavita , C. Fontanive , R. Gratton , K. Muzic , S. Desidera , B. Biller , A. Scholz , A. Sozzetti , V. Squicciarini

Brown dwarfs, which straddle the mass range between stars and planets, appear to be common both in the solar neighborhood and in star-forming regions. Their ubiquity makes the question of their origin an important one both for our…

天体物理学 · 物理学 2007-05-23 Ray Jayawardhana