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Table · dataset · 2026

SMGPS cross-matched with eROSITA/ROSAT and GaiaDR3

Listed in IVOA Registry (Virtual Observatory)

Radio emission from magnetically active stars arises primarily from non-thermal processes and provides information complementary to their high-energy X-ray emission.

Description

Recent advances in sensitive, wide-field radio and X-ray surveys have enabled the identification of larger samples of active stars across the Galaxy. We aim to identify and characterise radio and X-ray-emitting stars in the Galactic plane by combining MeerKAT radio data with soft X-ray observations, and to assess their consistency with the canonical Guedel-Benz relation, which states that the thermal coronal emission observed in soft X-rays is correlated with the non-thermal gyrosynchrotron emission detected in the radio.

We cross-matched compact radio sources from the SARAO MeerKAT Galactic Plane Survey with soft X-ray counterparts from the ROSAT All-Sky Survey and the first release of the SRG/eROSITA all-sky survey, the eRASS1. We investigated their radiobrightness temperatures and computed radio and X-ray luminosities to test for consistency with the Guedel-Benz relation. We identify 137 stellar sources with both radio and X-ray detections.

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Their radio-brightness temperatures, T_B_, range from 10^7^ to 10^12^K, with the exception of two outliers: AXJ1600.9-5142 (T_B_=4.8+/-1.5x10^12^K) and HD 124831 (T_B_=8+/-1x10^6^K). The remaining sources are consistent with emission from incoherent gyrosynchrotron processes. The sample generally lies below the canonical Guedel-Benz relation, with the offset predominantly driven by enhanced radio luminosities at 1.3GHz relative to the canonical relation derived at 5GHz.

Our results suggest that the classical Guedel-Benz relation represents an upper envelope rather than a tight correlation for active stars detected at 1.3GHz. In addition, the eROSITA detections show that early-type stars are systematically below the log(L_X_/L_bol_)~-3 relation, which is usually seen for stars of a later spectral type.

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Stated by source
Optical · Radio · X-Ray
Inferred from text
Astronomical sciences 71%
Provenance · 1 source records, 11 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/707/a19312 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].anzsrc:group:5101enrichment · IVOA Registrytaxonomy-embedding@1.1.0title+keywords+description (71%)
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:radiosource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:x-raysource · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0