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We report the detection of the likely companion of the binary millisecond pulsar J0740+6620 with the Gran Telescopio Canarias in the $r'$ and $i'$ bands. The position of the detected starlike source coincides with the pulsar coordinates…

太阳与恒星天体物理 · 物理学 2019-03-04 D. M. Beronya , A. V. Karpova , A. Yu. Kirichenko , S. V. Zharikov , D. A. Zyuzin , Yu. A. Shibanov , A. Cabrera-Lavers

A near-infrared excess is detected at the white dwarf PHL5038 in UKIDSS photometry, consistent with the presence of a cool, substellar companion. We have obtained H- and K-grism spectra and images of PHL5038 using NIRI on Gemini North. The…

太阳与恒星天体物理 · 物理学 2015-05-13 P. R. Steele , M. R. Burleigh , J. Farihi , B. T. Gaensicke , R. F. Jameson , P. D. Dobbie , M. A. Barstow

Through the Backyard Worlds: Planet 9 citizen science project we discovered a late-type L dwarf co-moving with the young K0 star BD+60 1417 at a projected separation of 37" or 1662 AU. The secondary - CWISER J124332.12+600126.2 (W1243) - is…

We report the results of an infrared Doppler survey designed to detect brown dwarf and giant planetary companions to a magnitude-limited sample of ultracool dwarfs. Using the NIRSPEC spectrograph on the Keck II telescope, we obtained…

太阳与恒星天体物理 · 物理学 2015-05-19 Cullen H. Blake , David Charbonneau , Russel J. White

We present Keck near-infrared imaging of three binary L dwarf systems, all of which are likely to be sub-stellar. Two are lithium dwarfs, and a third exhibits an L7 spectral type, making it the coolest binary known to date. All have…

天体物理学 · 物理学 2010-01-28 D. W. Koerner , J. Davy Kirkpatrick , M. W. McElwain , N. R. Bonaventura

We report the discovery of a high proper motion L subdwarf ($\mu$ =0.617arcsec/yr) in the Sloan Digital Sky Survey spectral database. The optical spectrum from the star SDSS J125637-022452 has mixed spectral features of both late-M spectral…

太阳与恒星天体物理 · 物理学 2009-11-13 T. Sivarani , S. Lépine , A. K. Kembhavi , J. Gupchup

We report the discovery of two faint ultracool companions to the nearby (d~17.9 pc) young G2V star HD 130948 (HR 5534, HIP 72567) using the Hokupa'a adaptive optics instrument mounted on the Gemini North 8-meter telescope. Both objects have…

天体物理学 · 物理学 2009-11-07 D. Potter , E. L. Martín , M. C. Cushing , P. Baudoz , W. Brandner , O. Guyon , R. Neuhauser

We present near-infrared magnitudes for all white dwarfs (selected from the catalog of McCook & Sion) contained in the 2 Micron All Sky Survey Second Incremental Data Release(2MASS 2IDR). We show that the near-IR color-color diagram is an…

We have used Pan-STARRS1 to discover an extremely red late-L dwarf, which has (J-K)_MKO = 2.84 and (J-K)_2MASS = 2.78, making it the reddest known field dwarf and second only to 2MASS J1207-39b among substellar companions. Near-IR…

While radial velocity surveys have demonstrated that the population of gas giants peaks around $3~\text{au}$, the most recent high-contrast imaging surveys have only been sensitive to planets beyond $\sim~10~\text{au}$. Sensitivity at small…

We report the tentative detection of the near-infrared emission of the Hot Jupiter WASP-12b with the low-resolution prism on IRTF/SpeX. We find a K-H contrast color of 0.137% +/- 0.054%, corresponding to a blackbody of temperature 2400…

地球与行星天体物理 · 物理学 2012-04-12 Ian J. M. Crossfield , Brad M. S. Hansen , Travis Barman

We present 2.9-4.1 micron integral field spectroscopy of the L4+L4 brown dwarf binary HD 130948BC, obtained with the Arizona Lenslets for Exoplanet Spectroscopy (ALES) mode of the Large Binocular Telescope Interferometer (LBTI). The HD…

The recently discovered star SCR 1845-6357 is the first late M/T dwarf binary discovered. SCR 1845 is a particular object due to its tight orbit (currently around 4 AU) and its proximity to the Sun (3.85 pc). We present spatially resolved…

天体物理学 · 物理学 2009-11-13 Markus Kasper , Beth A. Biller , Adam Burrows , Wolfgang Brandner , Jano Budaj , Laird M. Close

We report detection of the binary companion to the millisecond pulsar J2302+4442 based on the deep observations performed with the Gran Telescopio Canarias. The observations revealed an optical source with $r'$ = 23.33$\pm$0.02 and…

太阳与恒星天体物理 · 物理学 2018-08-08 A. Yu. Kirichenko , S. V. Zharikov , D. A. Zyuzin , Yu. A. Shibanov , A. V. Karpova , S. Dai , A. Cabrera-Lavers

Infrared excesses due to dusty disks have been observed orbiting white dwarfs with effective temperatures between 7200 K and 25000 K, suggesting that the rate of tidal disruption of minor bodies massive enough to create a coherent disk…

We present IRTF SpeX observations of the M/L binary system 2MASS J17072343-0558249. SpeX imaging resolves the system into a 1"01+/-0.17 visual binary in which both components have red near infrared colors. Resolved low-resolution (R~150)…

天体物理学 · 物理学 2008-11-26 Michael W. McElwain , Adam J. Burgasser

Brown dwarfs with known physical properties (e.g., age and mass) are essential for constraining models of the formation and evolution of substellar objects. We present new high-contrast imaging observations of the circumbinary brown dwarf…

地球与行星天体物理 · 物理学 2025-03-10 Gabriel Weible , Kevin Wagner , Jordan Stone , Steve Ertel , Dániel Apai , Kaitlin Kratter , Jarron Leisenring

Studying cold brown dwarfs is key to understanding the diverse characteristics of cold giant exoplanets atmospheres. COCONUTS-2, is a wide binary system composed of a T9 brown dwarf and an M3 star, which presents a unique opportunity to…

We present new imaging and spectroscopic data of the young Herbig star HD 144432 A, which was known to be a binary star with a separation of 1.47 arcsec. High-resolution NIR imaging data obtained with NACO at the VLT reveal that HD 144432 B…

太阳与恒星天体物理 · 物理学 2015-05-30 A. Mueller , A. Carmona , M. E. van den Ancker , R. van Boekel , Th. Henning , R. Launhardt