English
Related papers

Related papers: The very nearby M/T dwarf binary SCR 1845-6357

200 papers

Context. HD13724 is a nearby solar-type star at 43.48 $\pm$ 0.06 pc hosting a long-period low-mass brown dwarf detected with the CORALIE echelle spectrograph as part of the historical CORALIE radial-velocity search for extra-solar planets.…

Earth and Planetary Astrophysics · Physics 2020-04-06 E. L. Rickman , D. Ségransan , J. Hagelberg , J. -L. Beuzit , A. Cheetham , J. -B. Delisle , T. Forveille , S. Udry

We present the discovery of a white dwarf companion at 3.6" from GJ3346, a nearby ($\pi\sim$42 mas) K star observed with SPHERE@VLT as part of an open time survey for faint companions to objects with significant proper motion discrepancies…

Solar and Stellar Astrophysics · Physics 2020-03-04 M. Bonavita , C. Fontanive , S. Desidera , V. D'Orazi , A. Zurlo , K. Muzic , B. Biller , R. Gratton , D. Mesa , A. Sozzetti

The nearby Sun-like star HD 19467 shows a subtle radial velocity (RV) acceleration of -1.37+/-0.09 m/s/yr over an 16.9 year time baseline (an RV trend), hinting at the existence of a distant orbiting companion. We have obtained…

The masses and temperatures of young low mass stars and brown dwarfs in star- forming regions are not yet well established because of uncertainties in the age of individual objects and the spectral type vs. temperature scale appropriate for…

Astrophysics · Physics 2009-11-13 F. C. Riddick , P. F. Roche , P. W. Lucas

We present infrared H- and K-band spectra of a companion candidate 3" north of the young star GSC 08047-00232, a probable member of the nearby young Horologium association. From previously obtained JHK-band colors and the magnitude…

Astrophysics · Physics 2009-11-10 Ralph Neuhaeuser , Eike Guenther

We have completed a high-resolution (R=60,000) optical spectroscopic survey of 185 nearby M dwarfs identified using ROSAT data to select active, young objects with fractional X-ray luminosities comparable to or greater than Pleiades…

Solar and Stellar Astrophysics · Physics 2014-11-18 Evgenya Shkolnik , Michael C. Liu , I. Neill Reid

Hot subdwarfs in close binaries with either M dwarf, brown dwarf or white dwarf companions show unique light variations. In hot subdwarf binaries with M dwarf or brown dwarf companions we can observe the so-called reflection effect and in…

Solar and Stellar Astrophysics · Physics 2023-05-10 V. Schaffenroth , B. N. Barlow , I. Pelisoli , S. Geier , T. Kupfer

We present near-infrared spectra for a sample of T dwarfs, including eleven new discoveries made using the Two Micron All Sky Survey. These objects are distinguished from warmer (L-type) brown dwarfs by the presence of methane absorption…

We report on the discovery of the companion star to the millisecond pulsar J1342+2822B in the globular cluster M3. We exploited a combination of near-ultraviolet and optical observations acquired with the Hubble Space Telescope in order to…

High Energy Astrophysical Phenomena · Physics 2019-04-17 M. Cadelano , F. R. Ferraro , A. G. Istrate , C. Pallanca , B. Lanzoni , P. C. C. Freire

We report the discovery of EPIC 219388192 b, a transiting brown dwarf in a 5.3-day orbit around a member star of Ruprecht-147, the oldest nearby open cluster association, which was photometrically monitored by K2 during its Campaign 7. We…

We present a near-infrared spectrum of the hot ($T_{\rm eff}$ $\approx$ 55,000 K) DA white dwarf PG 1234+482. We confirm that a very low mass companion is responsible for the previously recognised infrared photometric excess. We compare…

Astrophysics · Physics 2009-11-13 P. R. Steele , M. R. Burleigh , P. D. Dobbie , M. A. Barstow

We report our discovery of an extremely rare, low mass, quadruple-lined spectroscopic binary BD-22 5866 (=NLTT 53279, integrated spectral type = M0 V), found during an ongoing search for the youngest M dwarfs in the solar neighborhood. From…

We report the discovery of a single-lined spectroscopic binary with an Ultra Cool Dwarf (UCD) primary with a spectral type between M8 and L0.5. This system was discovered during the course of an ongoing survey to monitor L dwarfs for radial…

We report the first direct detection of a strong, 5 kG magnetic field on the surface of an active brown dwarf. LSR J1835+3259 is an M8.5 dwarf exhibiting transient radio and optical emission bursts modulated by fast rotation. We have…

Solar and Stellar Astrophysics · Physics 2017-10-04 S. V. Berdyugina , D. M. Harrington , O. Kuzmychov , J. R. Kuhn , G. Hallinan , A. F. Kowalski , S. L. Hawley

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…

Solar and Stellar Astrophysics · Physics 2015-05-19 Cullen H. Blake , David Charbonneau , Russel J. White

We present i and z photometry for 25 T dwarfs and one L dwarf. Combined with published photometry, the data show that the i - z, z - Y and z - J colors of T dwarfs are very red, and continue to increase through to the late-type T dwarfs,…

We observed spectroscopically the eclipsing binary system T-Cyg1-01385 in order to determine physical properties of the components. The double-lined nature of the system is revealed for the first time and the radial velocities are obtained…

Solar and Stellar Astrophysics · Physics 2015-06-15 O. Cakirli , C. Ibanoglu , E. Sipahi

We report the discovery that the nearby ($\sim$ 6 pc) photometrically variable T2.5 dwarf SIMP~J013656.5+093347 is a likely member of the $\sim$ 200 Myr-old Carina-Near moving group with a probability of $>$ 99.9% based on its full…

Luhman and collaborators recently discovered an early-T dwarf companion to the G0 dwarf star HN Peg, using Spitzer Infrared Array Camera (IRAC) images. Companionship was established on the basis of the common proper motion inferred from…

NSVS 14256825 is the second sdOB + dM eclipsing binary systems with an orbital period of 2.65 hours. The special binary was reported to contain circumbinary planets or brown dwarfs by using the timing method. However, different results were…

Solar and Stellar Astrophysics · Physics 2020-04-01 Zhu L. -Y. , Qian S. -B. , Fernandez Lajus , E. , Wang Z. -H. , Li L. -J