Search Publications

Resolving Red Giant Winds with the Hubble Space Telescope
DOI: 10.3847/1538-4357/ad401f Bibcode: 2024ApJ...967..120W

Harper, Graham M.; Wood, Brian E.; Müller, Hans-Reinhard

We describe recent spectroscopic observations of red giant stars made by the Space Telescope Imaging Spectrograph (STIS) instrument on board the Hubble Space Telescope, which has provided spatially resolved observations of the warm chromospheric winds that predominate for early K to mid-M giants. The H I Lyα lines of a set of 11 red giants observe…

2024 The Astrophysical Journal
eHST 0
KIC 6362386: An Eclipsing Binary with γ Doradus–type Pulsations and Starspots
DOI: 10.3847/1538-3881/ad8913 Bibcode: 2024AJ....168..280J

Zhang, Xiaobin; Zong, Weikai; Wang, Jiaxin +5 more

KIC 6362386 is an eclipsing binary system that exhibits both γ Doradus (γ Dor)–type pulsations and starspots. In this study, we investigated this binary system using the Kepler photometry and the spectroscopic data from the Large Sky Area Multi-Object Fiber Spectroscopic Telescope. After employing the PHOEBE program for light-curve and radial-velo…

2024 The Astronomical Journal
Gaia 0
Primeros resultados del estudio observacional de estrellas masivas y centrales en cúmulos abiertos
Bibcode: 2024BAAA...65..102A

González, J. F.; Alejo, A. D.; González, S. P.

Theoretical models show that binary and multiple stars play an important rol in the energetics of open clusters and therefore in their dynamical evolution, particulary in poor clusters dominated by one or a few central massive stars. In this work we present the results of our spectroscopic, astrometric and photometric analysis of four young open c…

2024 Boletin de la Asociacion Argentina de Astronomia La Plata Argentina
Gaia 0
JWST Resolves Collision-induced Absorption Features in White Dwarfs
DOI: 10.3847/1538-4357/ad863b Bibcode: 2024ApJ...976..218B

Blouin, Simon; Dufour, Patrick; Kilic, Mukremin +2 more

Infrared-faint white dwarfs are cool white dwarfs exhibiting significant infrared flux deficits, most often attributed to collision-induced absorption (CIA) from H2–He in mixed hydrogen–helium atmospheres. We present James Webb Space Telescope (JWST) near- and mid-infrared spectra of three such objects using Near-Infrared Spectrograph (…

2024 The Astrophysical Journal
Gaia JWST 0
Solar Wind Turbulence and Complexity Probed with Rank-Ordered Multifractal Analysis (ROMA)
DOI: 10.3390/e26110929 Bibcode: 2024Entrp..26..929E

Voitcu, Gabriel; Echim, Marius; Munteanu, Costel +1 more

The Rank-Ordered Multifractal Analysis (ROMA) is a tool designed to characterize scale (in)variance and multifractality based on rank ordering the fluctuations in "groups" characterized by the same mono-fractal behavior (Hurst exponent). A range-limited structure-function analysis provides the mono-fractal index for each rank-ordered range of fluc…

2024 Entropy
Ulysses VenusExpress 0
Prolonged Fluvial Activity Revealed by Mapping and Analyses of Valley Networks in the Northwestern Hellas Region, Mars
DOI: 10.1029/2024JE008601 Bibcode: 2024JGRE..12908601X

Xiao, Long; Zhao, Jiannan; Shi, Yutong +4 more

Valley networks (VNs) on Mars are crucial for understanding the Martian hydrologic and climatic history. However, the limited resolution of remote sensing data hindered the complete identification of Martian VNs, affecting our understanding of the formation and duration of VNs as well as their climatic significance. In this study, we utilized high…

2024 Journal of Geophysical Research (Planets)
MEx 0
Observational Characteristics of Solar EUV Waves
DOI: 10.25518/0037-9565.11938 Bibcode: 2024BSRSL..93..962C

Joshi, Bhuwan; Chen, P. F.; Awasthi, Arun Kumar +4 more

Extreme-ultraviolet (EUV) waves are one of the large-scale phenomena on the Sun. They are defined as large propagating fronts in the low corona with speeds ranging from a few tens km s‑1 to several 1000 km s‑1. They are often associated with solar filament eruptions, flares, and/or coronal mass ejections (CMEs). EUV waves exhibit various features,…

2024 Bulletin de la Societe Royale des Sciences de Liege
SOHO 0
Chromospheric Mg I emission lines of pre-main-sequence stars
DOI: 10.1051/0004-6361/202452025 Bibcode: 2024A&A...691A.304Y

Itoh, Yoichi; Takagi, Yuhei; Yamashita, Mai

Context. To reveal details of the internal structure, the relationship between chromospheric activity and the Rossby number has been extensively examined for main-sequence stars. For active pre-main-sequence (PMS) stars, it is suggested that the level of activity be assessed using optically thin emission lines, such as Mg I. Aims. We aim to detect…

2024 Astronomy and Astrophysics
Gaia 0
Statistical Investigation of Wave Propagation in the Quiet-Sun Using IRIS Spectroscopic Observations
DOI: 10.3847/1538-4357/ad36ca Bibcode: 2024ApJ...966..187S

Srivastava, A. K.; Scullion, E.; Kayshap, P. +2 more

In this analysis, we use spectroscopic observations of the quiet Sun made by the IRIS instrument and investigate wave propagation. We analyze various spectral lines formed in different atmospheric layers, such as the photosphere, chromosphere, and transition region. We examine the Doppler velocity time series at various locations in the quiet Sun …

2024 The Astrophysical Journal
IRIS 0
Searching for planet-driven dust spirals in ALMA visibilities
DOI: 10.1093/mnras/stae1094 Bibcode: 2024MNRAS.530.4802S

Clarke, Cathie J.; Booth, Richard A.; Ribas, Álvaro +2 more

Atacama Large Millimetre/submillimetre Array (ALMA) observations of the thermal emission from protoplanetary disc dust have revealed a wealth of substructures that could evidence embedded planets, but planet-driven spirals, one of the more compelling lines of evidence, remain relatively rare. Existing works have focused on detecting these spirals …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 0