Search Results - "Guenther, E W"
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Properties of flares and CMEs on EV Lac: possible erupting filament
Published in Monthly notices of the Royal Astronomical Society (01-12-2020)“…ABSTRACT Flares and coronal mass ejections (CMEs) are very powerful events in which energetic radiation and particles are ejected within a short time. These…”
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2
Stellar coronal mass ejections – II. Constraints from spectroscopic observations
Published in Monthly notices of the Royal Astronomical Society (21-05-2020)“…ABSTRACT Detections of stellar coronal mass ejections (CMEs) are still rare. Observations of strong Balmer line asymmetries during flare events have been…”
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3
A census of coronal mass ejections on solar-like stars
Published in Monthly notices of the Royal Astronomical Society (01-04-2020)“…ABSTRACT Coronal mass ejections (CMEs) may have major importance for planetary and stellar evolution. Stellar CME parameters, such as mass and velocity, have…”
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4
A search for flares and mass ejections on young late-type stars in the open cluster Blanco-1
Published in Monthly notices of the Royal Astronomical Society (01-09-2014)“…We present a search for stellar activity (flares and mass ejections) in a sample of 28 stars in the young open cluster Blanco-1. We use optical spectra…”
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5
The flare-activity of 2MASS J16111534–1757214 in the upper Scorpius association
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT Flares are known to play an important role for the evolution of the atmospheres of young planets. In order to understand the evolution of planets, it…”
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6
Pre-main-sequence stars in the star-forming complex Sh 2-284
Published in Monthly notices of the Royal Astronomical Society (01-01-2011)“…Located at the Galactic anticentre, Sh 2-284 is an H ii region that harbours several young open clusters. Dolidze 25, a rare metal-poor (Z∼ 0.004) young…”
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Sub-stellar companions of intermediate-mass stars with CoRoT: CoRoT–34b, CoRoT–35b, and CoRoT–36b
Published in Monthly notices of the Royal Astronomical Society (27-08-2022)“…ABSTRACT Theories of planet formation give contradicting results of how frequent close-in giant planets of intermediate mass stars (IMSs; $1.3\le M_{\star }\le…”
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A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c
Published in Monthly notices of the Royal Astronomical Society (01-03-2024)“…ABSTRACT Ultra-short period planets (USPs) have orbital periods of less than 1 d. Since their masses and radii can be determined to a higher precision than…”
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9
Everything that glitters is not gold: V1315 Cas is not a dormant black hole
Published in Monthly notices of the Royal Astronomical Society (29-07-2023)“…ABSTRACT The quest for quiet or dormant black holes has been ongoing since several decades. Ellipsoidal variables possibly indicate the existence of a very…”
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10
The TWA 3 Young Triple System: Orbits, Disks, Evolution
Published in The Astrophysical journal (01-08-2017)“…We have characterized the spectroscopic orbit of the TWA 3A binary and provide preliminary families of probable solutions for the TWA 3A visual orbit, as well…”
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Spectral synthesis analysis and radial velocity study of the northern F-, G- and K-type flare stars
Published in Monthly notices of the Royal Astronomical Society (01-01-2006)“…In this paper, we present a study of the general physical and chemical properties and radial velocity monitoring of young active stars. We derive temperatures,…”
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12
MO Lup: a hierarchical triple T Tauri system
Published in Monthly notices of the Royal Astronomical Society (21-04-2007)“…In this paper, we present a thorough study of the T Tauri system MO Lup. We report on its previously unrecognized triple spectroscopic nature. Our study is…”
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13
K2-140b and K2-180b – Characterization of a hot Jupiter and a mini-Neptune from the K2 mission
Published in Monthly notices of the Royal Astronomical Society (11-01-2019)“…We report the independent discovery and characterization of two K2 planets: K2-180b, a mini-Neptune-sized planet in an 8.9-d orbit transiting a V = 12.6 mag,…”
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14
On the optimum operating conditions of ThNe calibration lamps for measurements of radial velocity variations
Published in Astronomische Nachrichten (01-06-2017)“…Previous studies have shown that ThNe lamps are very suitable for the precise measurement of wavelength variations. A critical issue for all hollow cathode…”
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15
The power of low-resolution spectroscopy: On the spectral classification of planet candidates in the ground-based CoRoT follow-up
Published in Astronomische Nachrichten (01-03-2015)“…Planetary transits detected by the CoRoT mission can be mimicked by a low‐mass star in orbit around a giant star. Spectral classification helps to identify the…”
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Flare stars in the TW Hydrae association: the HIP 57269 system
Published in Astronomische Nachrichten (01-11-2003)“…We discuss a new member candidate of the TW Hydrae association (TWA) among the stars of the Gershberg et al. (1999) flare star catalog. TWA is one of the…”
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17
A planet in a polar orbit of 1.4 solar-mass star
Published in EPJ Web of conferences (01-01-2015)“…Although more than a thousand transiting extrasolar planets have been discovered, only very few of them orbit stars that are more massive than the Sun. The…”
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Journal Article Conference Proceeding -
18
Hot subdwarfs in binary systems and the nature of their unseen companions
Published in Astrophysics and space science (01-10-2010)“…A large fraction of the sdB stars reside in short period binaries. It is therefore clear that binary evolution plays an important role in the still unsolved…”
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The Flare-Activity of 2MASSJ16111534-1757214 in the Upper Scorpius association
Published 24-06-2021“…Flares are known to play an important role for the evolution of the atmospheres of young planets. In order to understand the evolution of planets, it is thus…”
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Journal Article -
20
Stellar coronal mass ejections II. Constraints from spectroscopic observations
Published 08-05-2020“…MNRAS (2020) 494: 3766-3783 Detections of stellar coronal mass ejections (CMEs) are still rare. Observations of strong Balmer line asymmetries during flare…”
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