Showing 201 - 220 results of 300 for search '"brown dwarf"', query time: 0.13s Refine Results
  1. 201

    Three-dimensional SPH Simulations of FU Orionis Star Flares in the Clumpy Accretion Model by Tatiana V. Demidova, Vladimir P. Grinin

    Published 2023-01-01
    “…Such structures are usually associated with the existence in the vicinity of a star of a massive body (planet or brown dwarf), whose orbit is inclined relative to the plane of the disk. …”
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    Article
  2. 202

    Near-infrared InGaAs detectors for background-limited imaging and photometry by Sullivan, Peter W., Simcoe, Robert A., Croll, Bryce J.

    Published 2015
    “…InGaAs detectors are also applicable to other branches of near-infrared time-domain astronomy, ranging from brown dwarf weather to gravitational wave follow-up.…”
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    Article
  3. 203

    New low-mass eclipsing binary systems in Praesepe discovered by K2 by Gillen, E, Hillenbrand, L, David, T, Aigrain, S, Rebull, L, Stauffer, J, Cody, A, Queloz, D

    Published 2017
    “…The fourth system (AD 3116) comprises a brown dwarf transiting a mid M-dwarf, which is the first such system discovered in a sub-Gyr open cluster. …”
    Journal article
  4. 204

    The Gemini Deep Planet Survey by Lafreniere, D, Doyon, R, Marois, C, Nadeau, D, Oppenheimer, B, Roche, P, Rigaut, F, Graham, JR, Jayawardhana, R, Johnstone, D, Kalas, P, Macintosh, B, Racine, R

    Published 2007
    “…We present the results of the Gemini Deep Planet Survey, a near-infrared adaptive optics search for giant planets and brown dwarfs around 85 nearby young stars. The observations were obtained with the Altair adaptive optics sys- tem at the Gemini North telescope, and angular differential imaging was used to suppress the speckle noise of the central star. …”
    Journal article
  5. 205

    The Census of Exoplanets in Visual Binaries: Population Trends from a Volume-Limited Gaia DR2 and Literature Search by Clémence Fontanive, Daniella Bardalez Gagliuffi

    Published 2021-03-01
    “…We present results from an extensive search in the literature and Gaia DR2 for visual co-moving binary companions to stars hosting exoplanets and brown dwarfs within 200 pc. We found 218 planet hosts out of the 938 in our sample to be part of multiple-star systems, with 10 newly discovered binaries and 2 new tertiary stellar components. …”
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    Article
  6. 206

    Productivity of Three Dwarf Kopyor Coconut Varieties from Pati, Central Java, Indonesia by Ismail Maskromo, Sudarsono

    Published 2013-10-01
    “…Three varieties of Pati Dwarf Kopyor coconut, namely: Kopyor Green Dwarf, Kopyor Brown Dwarf and Kopyor Yellow Dwarf out of six potential varieties have been officially released as local superior varieties by the Minister of Agriculture, Republic of Indonesia at the end of 2010. …”
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    Article
  7. 207

    The Impact of Bayesian Hyperpriors on the Population-level Eccentricity Distribution of Imaged Planets by Vighnesh Nagpal, Sarah Blunt, Brendan P. Bowler, Trent J. Dupuy, Eric L. Nielsen, Jason J. Wang

    Published 2023-01-01
    “…Here, we study the effect of hyperpriors on the population-level eccentricity distributions inferred for the sample of directly imaged substellar companions (brown dwarfs and cold Jupiters) from hierarchical Bayesian modeling (HBM). …”
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    Article
  8. 208

    Sgr A* Spin and Mass Estimates through the Detection of an Extremely Large Mass-ratio Inspiral by Verónica Vázquez-Aceves, Yiren Lin, Alejandro Torres-Orjuela

    Published 2023-01-01
    “…In the present work, we show that detecting the gravitational waves (GWs) emitted by a brown dwarf inspiraling around Sgr A* will allow us to measure the mass and the spin of Sgr A* with unprecedented accuracy. …”
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    Article
  9. 209
  10. 210

    Subtle Signatures of Multiplicity in Late-type Dwarf Spectra: The Unresolved M8.5 + T5 Binary 2MASS J03202839–0446358 by Burgasser, Adam J., Liu, Michael C., Ireland, Michael J., Cruz, Kelle L., Dupuy, Trent J.

    Published 2011
    “…Evidence is presented that 2MASS J03202839–0446358, a late-type dwarf with discrepant optical (M8:) and near-infrared (L1) spectral types, is an as-yet unresolved stellar/brown dwarf binary with late-type M dwarf and T dwarf components. …”
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    Article
  11. 211

    Constraining the period of the ringed secondary companion to the young star J1407 with photographic plates by Mentel, RT, Kenworthy, MA, Cameron, DA, Scott, EL, Mellon, SN, Hudec, R, Birkby, JL, Mamajek, EE, Schrimpf, A, Reichart, DE, Haislip, JB, Kouprianov, VV, Hambsch, F-J, Tan, T-G, Hills, K, Grindlay, JE, Rodriguez, JE, Lund, MB, Kuhn, RB

    Published 2018
    “…These limits are still marginally consistent with a large Hill sphere filling ring system surrounding a brown dwarf companion in a bound elliptical orbit about J1407. …”
    Journal article
  12. 212

    The Gemini NICI Planet-Finding Campaign: The Frequency of Planets around Young Moving Group Stars by Biller, B, Liu, M, Wahhaj, Z, Nielsen, E, Hayward, T, Males, JR, Skemer, A, Close, L, Chun, M, Ftaclas, C, Clarke, F, Thatte, N, Shkolnik, E, Reid, I, Hartung, M, Boss, A, Lin, D, Alencar, S, Pino, E, Gregorio-Hetem, J, Toomey, D

    Published 2013
    “…Four co-moving companions of brown dwarf or stellar mass were discovered in this moving group sample: PZ Tel B (36+-6 MJup, 16.4+-1.0 AU, Biller et al. 2010), CD -35 2722B (31+-8 MJup, 67+-4 AU, Wahhaj et al. 2011), HD 12894B (0.46+-0.08 MSun, 15.7+-1.0 AU), and BD+07 1919C (0.20+-0.03 MSun, 12.5+-1.4 AU). …”
    Journal article
  13. 213

    The galaxy luminosity function at z ≃ 6 and evidence for rapid evolution in the bright end from z ≃ 7 to 5 by Bowler, R, Dunlop, J, McLure, R, McCracken, H, Milvang-Jensen, B, Furusawa, H, Taniguchi, Y, Le Fèvre, O, Fynbo, J, Jarvis, M, Häußler, B

    Published 2015
    “…We show that the expected contamination rate of our initial sample by cool Galactic brown dwarfs is ≲3 per cent and demonstrate that they can be effectively removed by fitting brown dwarf spectral templates to the photometry. …”
    Journal article
  14. 214

    Hot subdwarf stars in close-up view I. Rotational properties of subdwarf B stars in close binary systems and nature of their unseen companions by Geier, S, Heber, U, Podsiadlowski, P, Edelmann, H, Napiwotzki, R, Kupfer, T, Mueller, S

    Published 2010
    “…One binary may have a brown dwarf companion. The unseen companions of nine sdBs are white dwarfs with typical masses. …”
    Journal article
  15. 215

    Keragaan vegetatif dan generatif pada fase pembungaan awal kelapa Genjah kopyor asal kultur embrio di Bogor, Jawa Barat by M. Eko Riyo Bayu Prasetyo, Imron Riyadi, Sumaryono

    Published 2022-04-01
    “…When the first flowers appeared, Kopyor Brown Dwarf (KBD) had 14.6 fronds, while Kopyor Yellow Dwarf (KYD) and Kopyor Green Dwarf (KGD) had 15.5 and 17.1 fronds respectively. …”
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    Article
  16. 216

    KIC 7177553: A QUADRUPLE SYSTEM OF TWO CLOSE BINARIES by Lehmann, H., Borkovits, T., Ngo, H., Mawet, D., Csizmadia, Sz., Rappaport, Saul A., Forgacs-Dajka, E.

    Published 2016
    “…The implied mass of the third body is that of a super-Jupiter, but below the mass of a brown dwarf. We therefore embarked on a radial velocity (RV) study of this binary to determine its system configuration and to check the hypothesis that it hosts a giant planet. …”
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    Article
  17. 217

    Simultaneous Multiwavelength Variability Characterization of the Free-floating Planetary-mass Object PSO J318.5−22 by Biller, Beth A., Vos, Johanna, Buenzli, Esther, Allers, Katelyn, Bonnefoy, Mickaël, Charnay, Benjamin, Bézard, Bruno, Allard, France, Homeier, Derek, Bonavita, Mariangela, Brandner, Wolfgang, Crossfield, Ian Jm, Dupuy, Trent, Henning, Thomas, Kopytova, Taisiya, Liu, Michael C., Manjavacas, Elena, Schlieder, Joshua

    Published 2019
    “…We measure peak-to-trough variability amplitudes of 3.4% ± 0.1% for Spitzer Channel 2 and 4.4%-5.8% (typical 68% confidence errors of ∼0.3%) in the near-IR bands (1.07-1.67 μm) covered by the WFC3 G141 prism - the mid-IR variability amplitude for PSO J318.5-22 is one of the highest variability amplitudes measured in the mid-IR for any brown dwarf or planetary-mass object. Additionally, we detect phase offsets ranging from 200° to 210° (typical error of ∼4°) between synthesized near-IR light curves and the Spitzer mid-IR light curve, likely indicating depth-dependent longitudinal atmospheric structure in this atmosphere. …”
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    Article
  18. 218
  19. 219

    FUNDAMENTAL PROPERTIES OF KEPLER PLANET-CANDIDATE HOST STARS USING ASTEROSEISMOLOGY by Sanchis Ojeda, Roberto

    Published 2015
    “…Using the revised stellar properties, we recalculate the radii for 107 planet candidates in our sample, and comment on candidates for which the radii change from a previously giant-planet/brown-dwarf/stellar regime to a sub-Jupiter size or vice versa. …”
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    Article
  20. 220

    Exoplanet discoveries with the CoRoT space observatory by Lammer, H, Dvorak, R, Deleuil, M, Barge, P, Deeg, H, Moutou, C, Erikson, A, Csizmadia, S, Tingley, B, Bruntt, H, Havel, M, Aigrain, S, Almenara, J, Alonso, R, Auvergne, M, Baglin, A, Barbieri, M, Benz, W, Bonomo, A, Borde, P, Bouchy, F, Cabrera, J, Carone, L, Carpano, S, Ciardi, D

    Published 2010
    “…Discovered exoplanets such as CoRoT-3b populate the brown dwarf desert and close the gap of measured physical properties between usual gas giants and very low mass stars. …”
    Journal article