Search Publications

Kinematic study of the Orion Complex: analysing the young stellar clusters from big and small structures
DOI: 10.1093/mnras/stae2157 Bibcode: 2024MNRAS.534.2566S

Sánchez-Sanjuán, Sergio; Hernández, Jesús; Pérez-Villegas, Ángeles +4 more

In this work, we analysed young stellar clusters with spatial and kinematic coherence in the Orion star-forming complex. For this study, we selected a sample of pre-main-sequence candidates using parallaxes, proper motions, and positions on the colour-magnitude diagram. After applying a hierarchical clustering algorithm in the 5D parameter space p…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
Multi-spacecraft study with the Icarus model: Modelling the propagation of CMEs to Mercury and Earth
DOI: 10.1051/0004-6361/202450430 Bibcode: 2024A&A...689A..98B

Schmieder, B.; Poedts, S.; Démoulin, P. +2 more

Context. Coronal mass ejections (CMEs) are the main drivers of the disturbances in interplanetary space. Earth-directed CMEs can be dangerous, and understanding the CME interior magnetic structure is crucial for advancing space weather studies. It is important to assess the capabilities of a numerical heliospheric model, as a firm understanding of…

2024 Astronomy and Astrophysics
SOHO 1
Strong Effects of Chorus Waves on Radiation Belts Expected for Future Magnetic Superstorms
DOI: 10.1029/2024AV001234 Bibcode: 2024AGUA....501234S

Hanzelka, Miroslav; Santolík, Ondřej; Wang, Dedong +4 more

Processes in the radiation belts under extreme geomagnetic conditions involve the interplay between acceleration and loss processes, both of which can be caused by wave-particle interactions. Whistler mode waves play a critical role in these interactions, and up to now their properties during extreme events remained poorly sampled and understood. …

2024 AGU Advances
Cluster 1
CCD UBV(RI)KC photometry and dynamics of the open cluster NGC 1513
DOI: 10.1093/mnras/stae1237 Bibcode: 2024MNRAS.531.3715A

Akkaya Oralhan, İnci; Çakmak, Hikmet; Michel, Raúl +2 more

We derive astrophysical parameters of the open cluster NGC 1513 by means of colour indices built with new CCD UBV(RI)KC photometry. Based on early-type members, the mean foreground reddening and total to selective extinction ratio are E(B - V) = 0.79 ± 0.09 mag and RV = 2.85 ± 0.05. Through the differential grid method, we de…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
Multi-epoch X-ray spectral analysis of Centaurus A: Revealing new constraints on iron emission line origins
DOI: 10.1093/pasj/psae059 Bibcode: 2024PASJ...76..923I

Tanimoto, Atsushi; Bamba, Aya; Hagino, Kouichi +3 more

We conduct X-ray reverberation mapping and spectral analysis of the radio galaxy Centaurus A to uncover its central structure. We compare the light curve of the hard X-ray continuum from Swift Burst Alert Telescope observations with that of the Fe K$\alpha$ fluoresc…

2024 Publications of the Astronomical Society of Japan
Suzaku XMM-Newton 1
Lithium, rotation and metallicity in the open cluster M35
DOI: 10.1051/0004-6361/202450222 Bibcode: 2024A&A...687A.234C

Bouy, H.; Barrado, D.; Agüeros, M. A. +2 more

Context. Lithium (Li) abundance is an age indicator for G, K, and M stellar types, as its abundance decreases over time for these spectral types. However, despite all of the observational efforts made over the past few decades, the role of rotation, stellar activity, and metallicity in the depletion of Li is still unclear.
Aims: Our purpose i…

2024 Astronomy and Astrophysics
Gaia 1
JWST/NIRSpec Observations of Brown Dwarfs in the Orion Nebula Cluster
DOI: 10.3847/1538-4357/ad7b19 Bibcode: 2024ApJ...975..162L

Luhman, K. L.; Tremblin, P.; Parker, R. J. +4 more

We have used the multiobject mode of the Near-Infrared Spectrograph (NIRSpec) on board the James Webb Space Telescope (JWST) to obtain low-resolution 1–5 µm spectra of 22 brown dwarf candidates in the Orion Nebula Cluster, which were selected with archival images from the Hubble Space Telescope. One of the targets was previously classified a…

2024 The Astrophysical Journal
eHST JWST 1
Constraining the Excitation of Molecular Gas in Two Quasar-starburst Systems at z ∼ 6
DOI: 10.3847/1538-4357/ad8de2 Bibcode: 2024ApJ...977..190X

Fan, Xiaohui; Neri, Roberto; Menten, Karl M. +15 more

We present NOrthern Extended Millimeter Array observations of CO(8–7), (9–8), and (10–9) lines, as well as the underlying continuum for two far-infrared luminous quasars: SDSS J2054-0005 at z = 6.0389 and SDSS J0129-0035 at z = 5.7788. Both quasars were previously detected in CO (2–1) and (6–5) transitions, making them candidates for studying the …

2024 The Astrophysical Journal
Herschel 1
Latitudinal Mapping of Chorus Waves Growth Rates Based on Multi-Spacecraft Wave and Plasma Measurements
DOI: 10.1029/2024GL110539 Bibcode: 2024GeoRL..5110539V

Agapitov, O. V.; Artemyev, A.; Mourenas, D. +3 more

Whistler mode chorus waves are one of the most intense and important electromagnetic emissions in the Earth's radiation belt, where these waves are responsible for electron acceleration to relativistic energies and for energetic electron precipitation into the Earth's atmosphere. This study reports a unique multi-spacecraft observation event that …

2024 Geophysical Research Letters
Cluster 1
A comprehensive study of an oscillating eclipsing Algol: Y Camelopardalis
DOI: 10.1093/pasj/psae048 Bibcode: 2024PASJ...76..787C

Kahraman Aliçavuş, Filiz; Çelik, Eda

Y Camelopardalis (Y Cam) is classified as one of the oscillating eclipsing Algol (oEA) systems, which feature a $\delta$ Scuti-type pulsating component alongside mass transfer phenomena. oEA systems are invaluable for probing the evolutionary processes and internal structures of binary components, offering insights through their binary variations …

2024 Publications of the Astronomical Society of Japan
Gaia 1