Variable circularly polarized radio emission from the young stellar object [BHB2007]-1: Another ingredient of a unique system

The young stellar object [BHB2007]-1 has been extensively studied in the past at radio, millimeter, and infrared wavelengths. It has revealed a gap in the disk and previous observations have claimed possible emission from a sub-stellar object undergoing formation, in correspondence to the disk gap. In this work, we analyzed a set of eight Karl G. Jansky Very Large Array (VLA) observations at 15 GHz and spread out over a month. We inferred a slowly variable emission from the star, with a ∼15 − 20% circular polarization detected in two of the eight observations. The latter can be related to the magnetic fields in the system, while the unpolarized and moderately varying component can be indicative of free–free emission associated with jet induced shocks or interactions of the stellar wind, with dense surrounding material. We discarded any relevant short-flaring activities when sampling the radio light curves down to 10 seconds and found no clear evidence of emission from the sub-stellar object inferred from past observations, although deeper observations could shed further light on this.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2024-08-19
DOI
https://doi.org/10.1051/0004-6361/202450568
Citations
1
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.33

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article

Variable circularly polarized radio emission from the young stellar object [BHB2007]-1: Another ingredient of a unique system

T. Bhowmik, Daniele Viganò, Ó. Morata, Á. Sánchez-Monge et al.
1 citations
Astronomy and Astrophysics
Astro and Planetary Science
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article

Variable circularly polarized radio emission from the young stellar object [BHB2007]-1: Another ingredient of a unique system

T. Bhowmik, Daniele Viganò, Ó. Morata, Á. Sánchez-Monge, Simranpreet Kaur, A. Zurlo, J. M. Girart, L. Ilsedore Cleeves, F. O. Alves, Fabio Del Sordo
article en
1 citations

Abstract

The young stellar object [BHB2007]-1 has been extensively studied in the past at radio, millimeter, and infrared wavelengths. It has revealed a gap in the disk and previous observations have claimed possible emission from a sub-stellar object undergoing formation, in correspondence to the disk gap. In this work, we analyzed a set of eight Karl G. Jansky Very Large Array (VLA) observations at 15 GHz and spread out over a month. We inferred a slowly variable emission from the star, with a ∼15 − 20% circular polarization detected in two of the eight observations. The latter can be related to the magnetic fields in the system, while the unpolarized and moderately varying component can be indicative of free–free emission associated with jet induced shocks or interactions of the stellar wind, with dense surrounding material. We discarded any relevant short-flaring activities when sampling the radio light curves down to 10 seconds and found no clear evidence of emission from the sub-stellar object inferred from past observations, although deeper observations could shed further light on this.

Astronomy and AstrophysicsVol. 690
Institute of Space Sciences (ES), Institut d'Estudis Espacials de Catalunya (ES), Serviceplan (Germany) (DE), Institute of Space Sciences (ES), Osservatorio Astrofisico di Catania (IT), Millennium Engineering and Integration (United States) (US), Supply Chain Competence Center (Germany) (DE), Fundació Universitat-Empresa de les Illes Balears (ES), Govern de les Illes Balears (ES), Universitat de les Illes Balears (ES), University of Virginia (US), Universidad Diego Portales (CL)
European Space Agency, European Commission, Universitat Autònoma de Barcelona, Agencia Nacional de Investigación y Desarrollo, Agencia Estatal de Investigación, H2020 European Research Council
Openalex Percentile: Top 35%
Astro and Planetary Science
0.33
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