Search Publications

CHEOPS's hunt for exocomets: photometric observations of 5 Vul
DOI: 10.1093/mnras/stad1475 Bibcode: 2023MNRAS.523.1441R

Lecavelier Des Etangs, Alain; Zieba, Sebastian; Rebollido, Isabel +3 more

The presence of minor bodies in exoplanetary systems is in most cases inferred through infrared excesses, with the exception of exocomets. Even if over 35 yr have passed since the first detection of exocomets around β Pic, only ~25 systems are known to show evidence of evaporating bodies, and most of them have only been observed in spectroscopy. W…

2023 Monthly Notices of the Royal Astronomical Society
CHEOPS 3
Morpho-kinematic and photoionization models of the multipolar structures in planetary nebula NGC 6572
DOI: 10.1093/mnras/stad1897 Bibcode: 2023MNRAS.524.1547B

Parthasarathy, Mudumba; Das, Ramkrishna; Kar, Subhajit +1 more

We have studied planetary nebula (PN) NGC 6572 through 3D morpho-kinematic and photoionization modelling. The 3D morphology is reconstructed from the Hubble Space Telescope images in different narrow-band filters and position-velocity spectra. The PN has a multipolar morphology consisting of highly collimated outflows. The nebular image shows sign…

2023 Monthly Notices of the Royal Astronomical Society
eHST 3
Diving into the magnetosphere of the Of?p star HD 108
DOI: 10.1093/mnras/stad693 Bibcode: 2023MNRAS.521.2874R

Neiner, Coralie; Nazé, Yaël; Rauw, Gregor +1 more

We analyse optical and X-ray spectroscopy of the Of?p star HD 108, known for its strong dipolar magnetic field and its optical line profile variability with a time-scale of 54 ± 3 yrs, interpreted as the stellar rotation period. Optical emission lines have now recovered from their minimum emission state reached in 2007-2008. The variations of the …

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3
Influence of Intermittency on the Energy Transfer Rate of Solar Wind Turbulence
DOI: 10.3847/2041-8213/ad0a68 Bibcode: 2023ApJ...958L..28W

Wang, Xin; Yuan, Zhigang; Huang, Shiyong +2 more

The intermittency in the solar wind turbulence manifests itself in the anisotropic scaling due to the anisotropic spectral index and the intermittent level based on the extended P model. However, the influence of intermittency on the energy transfer rate remains unclear. Here we apply the partial variance of increments method to identify the inter…

2023 The Astrophysical Journal
Ulysses 3
The 3D kinematics of stellar substructures in the periphery of the Large Magellanic Cloud
DOI: 10.1093/mnras/stad1698 Bibcode: 2023MNRAS.523.4720N

Erkal, Denis; Belokurov, Vasily; Aguado, David S. +4 more

We report the 3D kinematics of 27 Mira-like stars in the northern, eastern, and southern periphery of the Large Magellanic Cloud (LMC), based on Gaia proper motions and a dedicated spectroscopic follow-up. Low-resolution spectra were obtained for more than 40 Mira-like candidates, selected to trace known substructures in the LMC periphery. Radial …

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3
The evolution of Martian fissure eruptions and their plumbing systems
DOI: 10.1016/j.epsl.2023.118382 Bibcode: 2023E&PSL.62118382P

Pieterek, Bartosz; Jones, Thomas J.

On Earth, the investigation of fissure eruptions and their deposits provide fundamental insights into the evolution of the subsurface volcanic plumbing system. On Mars, we have limited evidence of the spatiotemporal evolution of fissure-fed volcanic systems, and thus the processes operating within their subsurface-feeding dykes remain poorly under…

2023 Earth and Planetary Science Letters
MEx 3
IP Lyn: A Totally Eclipsing Contact Binary with an Extremely Low Mass Ratio
DOI: 10.1088/1674-4527/acd73c Bibcode: 2023RAA....23h5013Y

Meng, Zi-Bin; Yu, Yun-Xia; Hu, Ke +4 more

We present the first photometric and orbital period investigations for a neglected totally eclipsing contact binary IP Lyn. The photometric solutions derived from both ground-based and several surveys' observations suggest that it is a shallow contact binary with an extremely low mass ratio of 0.055. The weak asymmetry observed in our multiple ban…

2023 Research in Astronomy and Astrophysics
Gaia 3
High-velocity CP2 stars in the Galactic halo
DOI: 10.1051/0004-6361/202245464 Bibcode: 2023A&A...674A.215F

Paunzen, E.; Prišegen, M.; Faltová, N. +2 more

Context. The second subclass of chemically peculiar stars, the CP2 stars, are early-type stars exhibiting anomalous abundances with variable line strengths possibly also accompanied by photometric variability that typically belong to the Galactic disk. However, a small fraction of these objects were recently found to be located far from the Galact…

2023 Astronomy and Astrophysics
Gaia 3
Multiwavelength study of radio galaxy Pictor A: detection of western hotspot in far-UV and possible origin of high energy emissions
DOI: 10.1093/mnras/stad716 Bibcode: 2023MNRAS.521.2704G

Stalin, C. S.; Sreekumar, P.; Bhattacharya, Debbijoy +2 more

A comprehensive study of the nucleus and western hotspot of Pictor A is carried out using AstroSat observations, 13 yr of Fermi, and archival Swift observations along with other published data. We report the first detection of the western hotspot of Pictor A in the far-UV band using observations from AstroSat-UVIT. The broad-band SED of the wester…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3
Searching for quasi-periodic eruptions using machine learning
DOI: 10.1093/rasti/rzad015 Bibcode: 2023RASTI...2..238W

Young, A. J.; Webbe, Robbie

Quasi-periodic eruption (QPE) is a rare phenomenon in which the X-ray emission from the nuclei of galaxies shows a series of large amplitude flares. Only a handful of QPEs have been observed but the possibility remains that there are as yet undetected sources in archival data. Given the volume of data available a manual search is not feasible, and…

2023 RAS Techniques and Instruments
XMM-Newton 3