We present radio observations of 8 ultracool dwarfs with a narrow spectral type range (M8-M9.5) using the Very Large Array at 8.5 GHz. Only the tight M8 binary LP 349-25 was detected. LP 349-25 is the tenth ultracool dwarf system detected in radio and its trigonometric parallax pi = 67.6 mas, recently measured by Gatewood et al., makes it the furthest ultracool system detected by the Very Large Array to date, and the most radio-luminous outside of obvious flaring activity or variability
The Very Large Array was used to observe the ultracool rapidly rotating M9 dwarf TVLM 513-46546 simu...
We present milliarcsecond-resolution radio very long baseline interferometry (VLBI) observations of ...
Context. A selection of ultracool dwarfs are known to be radio active, with both gyrosynchrotron emi...
We present radio observations of eight ultracool dwarfs with a narrow spectral type range (M8-M9.5) ...
Context. A selection of ultracool dwarfs are known to be radio active, with both gyrosynchrotron emi...
Aims. With the purpose of investigating the radio emission of new ultracool objects, we carried out ...
Aims. With the purpose of investigating the radio emission of new ultracool objects, we carried out ...
Aims. We aim to increase the sample of ultracool dwarfs studied in the radio domain to allow a more ...
Aim. With the purpose of investigating the radio emission of new ultracool objects, we carried out a...
Ultracool dwarfs, the least-massive contributors to the stellar mass function, exhibit striking magn...
The well-studied M9 dwarf TVLM 513–46546 is a rapid rotator (P rot ~ 2 hr) hosting a stable, dipolar...
We report the results of a volume-limited survey using the Australia Telescope Compact Array to sear...
We report the detection of radio emission from the unusually active L5e + T7 binary 2MASS J13153094−...
We have used the VLA to conduct a deep search for 3.6 cm radio emission from nearby very low mass st...
We present multi-epoch radio and optical observations of the M7 dwarf 2MASS J13142039+1320011. We de...
The Very Large Array was used to observe the ultracool rapidly rotating M9 dwarf TVLM 513-46546 simu...
We present milliarcsecond-resolution radio very long baseline interferometry (VLBI) observations of ...
Context. A selection of ultracool dwarfs are known to be radio active, with both gyrosynchrotron emi...
We present radio observations of eight ultracool dwarfs with a narrow spectral type range (M8-M9.5) ...
Context. A selection of ultracool dwarfs are known to be radio active, with both gyrosynchrotron emi...
Aims. With the purpose of investigating the radio emission of new ultracool objects, we carried out ...
Aims. With the purpose of investigating the radio emission of new ultracool objects, we carried out ...
Aims. We aim to increase the sample of ultracool dwarfs studied in the radio domain to allow a more ...
Aim. With the purpose of investigating the radio emission of new ultracool objects, we carried out a...
Ultracool dwarfs, the least-massive contributors to the stellar mass function, exhibit striking magn...
The well-studied M9 dwarf TVLM 513–46546 is a rapid rotator (P rot ~ 2 hr) hosting a stable, dipolar...
We report the results of a volume-limited survey using the Australia Telescope Compact Array to sear...
We report the detection of radio emission from the unusually active L5e + T7 binary 2MASS J13153094−...
We have used the VLA to conduct a deep search for 3.6 cm radio emission from nearby very low mass st...
We present multi-epoch radio and optical observations of the M7 dwarf 2MASS J13142039+1320011. We de...
The Very Large Array was used to observe the ultracool rapidly rotating M9 dwarf TVLM 513-46546 simu...
We present milliarcsecond-resolution radio very long baseline interferometry (VLBI) observations of ...
Context. A selection of ultracool dwarfs are known to be radio active, with both gyrosynchrotron emi...