Search Publications

Two successive EUV waves and a transverse oscillation of a quiescent prominence
DOI: 10.1093/mnras/stae1936 Bibcode: 2024MNRAS.533.3255Z

Li, Y.; Yan, X. L.; Zhang, Q. M. +4 more

In this paper, we carry out multiwavelength observations of two successive extreme-ultraviolet (EUV) waves originating from active region (AR) NOAA 13575 and a transverse oscillation of a columnar quiescent prominence on 2024 February 9. A hot channel eruption generates an X3.4 class flare and the associated full-halo coronal mass ejection (CME), …

2024 Monthly Notices of the Royal Astronomical Society
SOHO 7
Evidence for Primordial Alignment: Insights from Stellar Obliquity Measurements for Compact Sub-Saturn Systems
DOI: 10.3847/1538-3881/ad61d8 Bibcode: 2024AJ....168..116R

Rice, Malena; Wang, Songhu; Wang, Xian-Yu +5 more

Despite decades of effort, the mechanisms by which the spin axis of a star and the orbital axes of its planets become misaligned remain elusive. In particular, it is of great interest whether the large spin–orbit misalignments observed are driven primarily by high-eccentricity migration—expected to have occurred for short-period, isolated planets—…

2024 The Astronomical Journal
Gaia 7
Structure formation with primordial black holes to alleviate early star formation tension revealed by JWST
DOI: 10.1051/0004-6361/202449565 Bibcode: 2024A&A...685L...8C

Padilla, N.; Colazo, P. E.; Stasyszyn, F.

Context. This Letter explores the potential role of primordial black holes (PBHs) to address cosmological tensions as the presence of more massive than expected galaxies at high redshifts, as indicated by recent James Webb Space Telescope observations.
Aims: Motivated by inflation models that enhance the power at scales beyond the observable …

2024 Astronomy and Astrophysics
JWST 7
The Environments of Fast Radio Bursts Viewed Using Adaptive Optics
DOI: 10.3847/1538-4357/ad643c Bibcode: 2024ApJ...973...64W

Kilpatrick, Charles D.; Simha, Sunil; Prochaska, J. Xavier +10 more

We present observations from the Gemini Multi-Conjugate Adaptive Optics System/Gemini South Adaptive Optics Imager at Gemini South of five fast radio burst (FRB) host galaxies of FRBs with subarcsecond localizations. We examine and quantify the spatial distributions and locations of the FRBs with respect to their host galaxy light distributions, f…

2024 The Astrophysical Journal
eHST 7
Modeling JWST MIRI-MRS Observations of T Cha: Mid-IR Noble Gas Emission Tracing a Dense Disk Wind
DOI: 10.3847/1538-3881/ad34ae Bibcode: 2024AJ....167..223S

Pascucci, Ilaria; Gorti, Uma; Clarke, Cathie J. +8 more

[Ne II] 12.81 µm emission is a well-used tracer of protoplanetary disk winds due to its blueshifted line profile. Mid-Infrared Instrument (MIRI)-Medium Resolution Spectrometer (MRS) recently observed T Cha, detecting this line along with lines of [Ne III], [Ar II], and [Ar III], with the [Ne II] and [Ne III] lines found to be extended while …

2024 The Astronomical Journal
Gaia 7
Ultra-low-frequency LOFAR spectral indices of cluster radio halos
DOI: 10.1051/0004-6361/202450697 Bibcode: 2024A&A...689A.218P

Di Gennaro, G.; Brunetti, G.; Tasse, C. +12 more

Context. A fraction of galaxy clusters harbor diffuse radio sources known as radio halos. The prevailing theory regarding their formation is based on second-order Fermi reacceleration of seed electrons caused by merger-driven turbulence in the intra-cluster medium. This mechanism is expected to be inefficient, which implies that a significant frac…

2024 Astronomy and Astrophysics
XMM-Newton 7
Star-formation activity of low-mass galaxies at the peak epoch of galaxy formation probed by deep narrow-band imaging
DOI: 10.1093/mnras/stae1243 Bibcode: 2024MNRAS.531.2335D

Suzuki, Tomoko L.; Koyama, Yusei; Kodama, Tadayuki +5 more

Low-mass galaxies at high redshifts are the building blocks of more massive galaxies at later times and are thus key populations for understanding galaxy formation and evolution. We have made deep narrow-band observations for two protoclusters and the general field in COSMOS at z ~ 2. In a clumpy young protocluster, USS1558-003, at z = 2.53, we fi…

2024 Monthly Notices of the Royal Astronomical Society
eHST 7
Flares confirmed for the first time to be from the primary component of an eclipsing binary
DOI: 10.1093/mnras/stad3251 Bibcode: 2024MNRAS.527.3982L

Li, Kai; Gao, Xing; Sun, Guo-You +3 more

Only a handful of precise observations of flare detected from a contact binary so far. This paper presents the photometric and spectroscopic analysis of a contact binary (ASAS J082243+1927.0). Two flare events detected from this object were observed in the data of TESS. The two flare events both occurred at the secondary minimum. Considering the t…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS
DOI: 10.1051/0004-6361/202348147 Bibcode: 2024A&A...683A.192J

Trifonov, Trifon; Henning, Thomas; Triaud, Amaury H. M. J. +48 more

We report on the confirmation and follow-up characterization of two long-period transiting substellar companions on low-eccentricity orbits around TIC 4672985 and TOI-2529, whose transit events were detected by the TESS space mission. Ground-based photometric and spectroscopic follow-up from different facilities, confirmed the substellar nature of…

2024 Astronomy and Astrophysics
Gaia 7
How Gaia sheds light on the Milky Way star cluster population
DOI: 10.1016/j.newar.2024.101696 Bibcode: 2024NewAR..9901696C

Casamiquela, L.; Cantat-Gaudin, T.

Star clusters are among the first celestial objects catalogued by early astronomers. As simple and coeval populations, their study has been instrumental in charting the properties of the Milky Way and providing insight into stellar evolution through the 20th century. Clusters were traditionally spotted as local stellar overdensities in the plane o…

2024 New Astronomy Reviews
Gaia 7