Search Results - "Robrade, J"
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A scaling relationship for non-thermal radio emission from ordered magnetospheres: from the top of the main sequence to planets
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT In this paper, we present the analysis of incoherent non-thermal radio emission from a sample of hot magnetic stars, ranging from early-B to early-A…”
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2
Coronal and Chromospheric Emission in A-type Stars
Published in The Astronomical journal (01-07-2022)“…Abstract Cool stars on the main sequence generate X-rays from coronal activity, powered by a convective dynamo. With increasing temperature, the convective…”
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Evidence for radio and X-ray auroral emissions from the magnetic B-type star ρ Oph A
Published in Monthly notices of the Royal Astronomical Society (21-04-2020)“…Abstract We present new ATCA multiwavelength radio measurements (range 2.1–21.2 GHz) of the early-type magnetic star ρ Oph A, performed in 2019 March during…”
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Proxima Centauri – the nearest planet host observed simultaneously with AstroSat, Chandra, and HST
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT Our nearest stellar neighbour, Proxima Centauri, is a low-mass star with spectral type dM5.5 and hosting an Earth-like planet orbiting within its…”
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The auroral radio emission of the magnetic B-type star ρ OphC
Published in Monthly notices of the Royal Astronomical Society. Letters (01-11-2020)“…ABSTRACT The non-thermal radio emission of main-sequence early-type stars is a signature of stellar magnetism. We present multiwavelength (1.6–16.7 GHz) ATCA…”
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Discovery and origin of the radio emission from the multiple stellar system KQ Vel
Published in Monthly notices of the Royal Astronomical Society (18-08-2022)“…ABSTRACT KQ Vel is a binary system composed of a slowly rotating magnetic Ap star with a companion of unknown nature. In this paper, we report the detection of…”
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Stellar X‐ray accretion signatures
Published in Astronomische Nachrichten (01-03-2017)“…Accretion is observed in a wide range of objects with partially overlapping properties. In this paper, we focus on accretion in young stars. Material impacting…”
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MN Lup: X-RAYS FROM A WEAKLY ACCRETING T TAURI STAR
Published in The Astrophysical journal (01-07-2013)“…Young T Tauri stars (TTS) are surrounded by an accretion disk, which over time disperses due to photoevaporation, accretion, and possibly planet formation. The…”
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SOFT CORONAL X-RAYS FROM β PICTORIS
Published in The Astrophysical journal (01-05-2012)“…A-type stars are expected to be X-ray dark, yet weak emission has been detected from several objects in this class. We present new Chandra/HRC-I observations…”
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10
Cool, warm and hot outflows from CTTS: The FUV view of DG Tau
Published in EPJ Web of conferences (2014)“…Classical T Tauri stars (CTTSs) drive strong outflows with temperatures from about 103 K up to a few 106 K. These outflows regulate the angular momentum…”
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SOFT CORONAL X-RAYS FROM {beta} PICTORIS
Published in The Astrophysical journal (01-05-2012)“…A-type stars are expected to be X-ray dark, yet weak emission has been detected from several objects in this class. We present new Chandra/HRC-I observations…”
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12
Cool, warm and hot outflows from CTTS: The FUV view of DG Tau
Published in EPJ Web of conferences (01-01-2014)“…Classical T Tauri stars (CTTSs) drive strong outflows with temperatures from about 10 super(3) K up to a few 10 super(6) K. These outflows regulate the angular…”
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13
The high-energy environment of the heavy sub-Earth GJ 367 b indicates likely complete evaporation of its atmosphere
Published 01-08-2024“…A&A 689, A188 (2024) The planet GJ 367 b is a recently discovered high-density sub-Earth orbiting an M dwarf star. Its composition was modelled to be…”
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The SRG/eROSITA all-sky survey -- Identifying the coronal content with HamStar
Published 30-01-2024“…The first eROSITA all-sky survey (eRASS1) performed on board the Spectrum-Roentgen-Gamma mission (SRG) provides more than 900,000 X-ray sources in the 0.2 -…”
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''Forbidden" stars in the eROSITA all-sky survey: X-ray emission from very late-type giants
Published 30-01-2024“…A&A 688, A9 (2024) We present the results of the first X-ray all-sky survey (eRASS1) performed by the eROSITA instrument onboard the Spectrum-Roentgen-Gamma…”
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eROSITA X-ray scan of the eta Chamaeleontis cluster
Published 28-06-2021“…The nearby young open cluster eta Chamaeleontis has been observed by eROSITA/SRG during its CalPV phase for 150 ks. The eROSITA data were taken in the…”
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The eROSITA DR1 variability catalogue
Published 30-01-2024“…The extended ROentgen Survey with an Imaging Telescope Array (eROSITA) on board the Spectrum-Roentgen-Gamma (SRG) mission with its first All-Sky Survey…”
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SRG/eROSITA 3D mapping of the ISM using X-ray absorption spectroscopy
Published 30-01-2024“…A&A 688, A207 (2024) We present a detailed study of the hydrogen density distribution in the local interstellar medium (ISM) using the X-ray absorption…”
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The stellar content of the ROSAT all-sky survey
Published 25-05-2022“…A&A 664, A105 (2022) We present and apply a method to identify the stellar content of the ROSAT all-sky survey (RASS). We performed a crossmatch between the…”
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Coronal and chromospheric emission in A-type stars
Published 12-05-2022“…Cool stars on the main sequence generate X-rays from coronal activity, powered by a convective dynamo. With increasing temperature, the convective envelope…”
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