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This paper reports Giant Metrewave Radio Telescope (GMRT) observations of the binary system HD 41004 that are among the deepest images ever obtained at 150~MHz and 400 MHz in the search for radio emission from exoplanets. The HD 41004…

We present the detection of the binary system 2MASS J02132062+3648506 AB using the Karl G. Jansky Very Large Array (VLA) archive data observed at 4-8 GHz. The system is a triple consisting of a tight binary ($\sim0.2"$) of two M dwarfs of…

With the improvements in radio interferometry sensitivity, the quest for coherent radio emission from exoplanets and ultra-cool dwarfs, which is indicative of their magnetic fields, has gained significant momentum in recent years. We…

Recent observations with the LOw Frequency ARray (LOFAR) have revealed 19 nearby M dwarfs showing bright circularly polarised radio emission. One of the possible sources of such emission is through magnetic star-planet interactions (MSPI)…

We report the discovery of two binary M dwarf systems in the immediate solar neighborhood using 2MASS. The first is an M6.5 companion to the nearby G star HD 86728 (Gl 376). The known properties of HD 86728 indicate that the M dwarf (Gl…

Astrophysics · Physics 2007-05-23 J. E. Gizis , D. G. Monet , I. N. Reid , J. D. Kirkpatrick , A. J. Burgasser

Radio observations of stars trace the plasma conditions and magnetic field properties of stellar magnetospheres and coronae. Depending on the plasma conditions at the emitter site, radio emission in the metre- and decimetre-wave bands is…

Solar and Stellar Astrophysics · Physics 2023-12-13 Timothy W. H. Yiu , Harish K. Vedantham , Joseph R. Callingham , Maximilian N. Günther

We present the serendipitous discovery of 8 distant ($>$ 50 pc) late M dwarfs with plausible associated radio emission at 144 MHz. The M dwarf nature of our sources has been confirmed with optical spectroscopy performed using HET/LRS2 and…

Brown dwarfs display Jupiter-like auroral phenomena such as magnetospheric H$\alpha$ emission and coherent radio emission. Coherent radio emission is a probe of magnetospheric acceleration mechanisms and provides a direct measurement of the…

Solar and Stellar Astrophysics · Physics 2023-07-12 H. K. Vedantham , Trent J. Dupuy , E. L. Evans , A. Sanghi , J. R. Callingham , T. W. Shimwell , W. M. J. Best , M. C. Liu , P. Zarka

Several binary systems that contain a massive star have been detected in both the radio band and at very high energies. In the dense stellar photon field of these sources, gamma-ray absorption and pair creation are expected to occur, and…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Valenti Bosch-Ramon , Dmitry Khangulyan

We report on a study of 36 pairs of `twin' M dwarfs in wide binaries and assess how similarly the stars behave. Stars in each twin pair have BP, RP, $J$, $H$, and $K_s$ differing by $<$0.10 mag, mass estimates matching within $<$3%, and…

Solar and Stellar Astrophysics · Physics 2026-02-18 Andrew A. Couperus , Todd J. Henry , Aman Kar , Wei-Chun Jao , Eliot Halley Vrijmoet , Rachel A. Osten

In order to understand the possible mechanisms of recurrent jet activity in radio galaxies and quasars, which are still unclear, we have identified such sources with a large range of linear sizes (220 $-$ 917 kpc), and hence time scales of…

Astrophysics of Galaxies · Physics 2019-07-17 S. Nandi , D. J. Saikia , R. Roy , P. Dabhade , Y. Wadadekar , J. Larsson , M. Baes , H. C. Chandola , M. Singh

Long period radio transients (LPTs) are the slowest radio-pulsing sources ever found, with the current population spanning periods of seven minutes to over six hours. Two of the thirteen published LPTs, ILT J1101+5521 and GLEAM-X J0704--37,…

Solar and Stellar Astrophysics · Physics 2026-04-22 Antonio C. Rodriguez , Kareem El-Badry , Iris de Ruiter , Kaustubh Rajwade , Edo Berger , Liam Connor , Natasha Hurley-Walker

We search for radio emission from star-planet interactions in the M-dwarf system GJ~486, which hosts an Earth-like planet. We observed the GJ~486 system with the upgraded Giant Metrewave Radio Telescope (uGMRT) from 550 to 750 MHz in nine…

We report new infrared radial velocity measurements obtained with CSHELL at NASA's Infrared Telescope Facility that reveal the M3.5 dwarf GJ 867B to be a single-lined spectroscopic binary with a period of 1.795 $\pm$ 0.017 days. Its…

Aims. With the aim to reveal the effects of the magnetic field to the multi-band activity of dwarf stars, we search for associated radio emission for an extensive list of 14 915 brown dwarfs and 15 124 flaring stars. Methods. We utilised…

Solar and Stellar Astrophysics · Physics 2025-06-30 K. Perger , B. Seli , K. Vida

The nature of two recently discovered radio emitters with unusually long periods of 18min (GLEAM-X J1627-52) and 21min (GPM J1839-10) is highly debated. Their bright radio emission resembles that of radio magnetars, but their long…

Radio emission has been detected from tens of white dwarfs, in particular in accreting systems. Additionally, radio emission has been predicted as a possible outcome of a planetary system around a white dwarf. We searched for 3 GHz radio…

We identify a sample of near-equal mass wide binary M dwarf systems from the SLoWPoKES catalog of common proper-motion binaries and obtain follow-up observations of their chromospheric activity as measured by the H$\alpha$ emission line. We…

Solar and Stellar Astrophysics · Physics 2015-06-23 Heather C. Gunning , Sarah J. Schmidt , James R. A. Davenport , Saurav Dhital , Suzanne L. Hawley , Andrew A. West

We present Very Large Array observations of twelve late M and L dwarfs in the Solar neighborhood. The observed sources were chosen to cover a wide range of physical characteristics - spectral type, rotation, age, binarity, and X-ray and…

Astrophysics · Physics 2009-11-07 E. Berger

With the purpose to investigate the radio emission of new ultracool objects, we carried out a targeted search in the recently discovered system VHS J125601.92$-$125723.9 (hereafter VHS 1256$-$1257); this system is composed by an equal-mass…

Solar and Stellar Astrophysics · Physics 2018-02-21 J. C. Guirado , R. Azulay , B. Gauza , M. A. Pérez-Torres , R. Rebolo , J. B. Climent , M. R. Zapatero-Osorio
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