A LOFAR detection of the low mass young star T Tau at 149 MHz - INSU - Institut national des sciences de l'Univers Access content directly
Journal Articles The Astrophysical Journal Year : 2017

A LOFAR detection of the low mass young star T Tau at 149 MHz

Sera Markoff

Abstract

Radio observations of young stellar objects (YSOs) enable the study of ionised plasma outflows from young protostars via their free–free radiation. Previous studies of the low-mass young system T Tau have used radio observations to model the spectrum and estimate important physical properties of the associated ionised plasma (local electron density, ionised gas content and emission measure). However, without an indication of the low-frequency turnover in the free–free spectrum, these properties remain difficult to constrain. This paper presents the detection of T Tau at 149 MHz with the Low Frequency Array (LOFAR)-the first time a YSO has been observed at such low frequencies. The recovered total flux indicates that the free–free spectrum may be turning over near 149 MHz. The spectral energy distribution is fitted and yields improved constraints on local electron density ((7.2 ± 2.1) × 10 3 cm −3), ionised gas mass ((1.0 ± 1.8) × 10 −6 M ⊙) and emission measure ((1.67 ± 0.14) × 10 5 pc cm −6).
Fichier principal
Vignette du fichier
1611.03282.pdf (593.46 Ko) Télécharger le fichier
Origin : Files produced by the author(s)
Loading...

Dates and versions

insu-01526723 , version 1 (23-05-2017)

Licence

Attribution - NonCommercial - NoDerivatives - CC BY 4.0

Identifiers

Cite

Colm P. Coughlan, Rachael E. Ainsworth, Jochen Eislöffel, Matthias Hoeft, Alexander Drabent, et al.. A LOFAR detection of the low mass young star T Tau at 149 MHz. The Astrophysical Journal, 2017, 834 (2), 206 (10 p.). ⟨10.3847/1538-4357/834/2/206⟩. ⟨insu-01526723⟩
3114 View
260 Download

Altmetric

Share

Gmail Facebook Twitter LinkedIn More