Search Publications

Kepler main-sequence solar-like stars: surface rotation and magnetic-activity evolution
DOI: 10.3389/fspas.2024.1356379 Bibcode: 2024FrASS..1156379S

García, Rafael A.; Breton, Sylvain N.; Mathur, Savita +4 more

While the mission's primary goal was focused on exoplanet detection and characterization, Kepler made and continues to make extraordinary advances in stellar physics. Stellar rotation and magnetic activity are no exceptions. Kepler allowed for these properties to be determined for tens of thousands of stars from the main sequence up to the red gia…

2024 Frontiers in Astronomy and Space Sciences
Gaia 7
The cool brown dwarf Gliese 229 B is a close binary
DOI: 10.1038/s41586-024-08064-x Bibcode: 2024Natur.634.1070X

Lutz, D.; Förster Schreiber, N. M.; Genzel, R. +76 more

Owing to their similarities with giant exoplanets, brown dwarf companions of stars provide insights into the fundamental processes of planet formation and evolution. From their orbits, several brown dwarf companions are found to be more massive than theoretical predictions given their luminosities and the ages of their host stars1–3. Ei…

2024 Nature
Gaia 7
Constraints on supermassive black hole binaries from JWST and NANOGrav
DOI: 10.1051/0004-6361/202449185 Bibcode: 2024A&A...684L..15P

Loeb, Abraham; Padmanabhan, Hamsa

We use the recent statistics of dual active galactic nuclei (AGN) in the James Webb Space Telescope (JWST) data at z ∼ 3.4 to address two aspects of the feedback and evolution scenarios of supermassive black hole binaries. We find that the JWST data provide evidence for the members of a binary BH being `lit' at the same time, rather than independe…

2024 Astronomy and Astrophysics
JWST 7
JWST COMPASS: The 3–5 µm Transmission Spectrum of the Super-Earth L 98-59 c
DOI: 10.3847/1538-3881/ad73cf Bibcode: 2024AJ....168..276S

Batalha, Natalie M.; Moran, Sarah E.; Kirk, James +14 more

We present a JWST Near-InfraRed Spectrograph (NIRSpec) transmission spectrum of the super-Earth exoplanet L 98-59 c. This small (R p = 1.385 ± 0.085R , M p = 2.22 ± 0.26 R ), warm (T eq = 553 K) planet resides in a multiplanet system around a nearby, bright (J = 7.933) M3V star. We find …

2024 The Astronomical Journal
JWST 7
Determining stellar accretion rates from Paα and Brβ emission lines with JWST NIRSpec. Accretion of pre-main-sequence stars in NGC 3603
DOI: 10.1051/0004-6361/202449282 Bibcode: 2024A&A...684L...8R

de Marchi, Guido; Brandl, Bernhard; Rogers, Ciarán

In this Letter, we present the first systematic spectroscopic measurements of the near-infrared (NIR) hydrogen recombination lines Paschen alpha (Paαλ = 1.875 µm) and Brackett beta (Brβλ = 2.626 µm), produced by pre-main-sequence (PMS) stars. Such stars include T Tauri and Herbig AeBe stars, located in the massive…

2024 Astronomy and Astrophysics
JWST 7
Clues to growth and disruption of two neighbouring spiral arms of the Milky Way
DOI: 10.1093/mnras/stae2041 Bibcode: 2024MNRAS.533.4324F

Matsunaga, Noriyuki; Kawata, Daisuke; Taniguchi, Daisuke +3 more

Studying the nature of spiral arms is essential for understanding the formation of the intricate disc structure of the Milky Way. The European Space Agency's Gaia mission has provided revolutionary observational data that have uncovered detailed kinematical features of stars in the Milky Way. However, so far the nature of spiral arms continues to …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
DOI: 10.3847/1538-4357/ad234a Bibcode: 2024ApJ...964...94C

Cleri, Nikko J.; Giavalisco, Mauro; Ji, Zhiyuan +3 more

We explore the relationships between the [O/H] gas-phase metallicity radial gradients and multiple galaxy properties for 238 star-forming galaxies at 0.6 < z < 2.6 selected from the CANDELS Lyα Emission at Reionization survey with stellar mass $8.5\lt \mathrm{log}\,{M}_{* }/{M}_{\odot }\lt 10.5$ . The gradients cover the range from ‑0.11 to …

2024 The Astrophysical Journal
eHST 7
CHEX-MATE: A LOFAR pilot X-ray - radio study on five radio halo clusters
DOI: 10.1051/0004-6361/202347965 Bibcode: 2024A&A...686A...5B

Brunetti, G.; Pointecouteau, E.; Pratt, G. W. +24 more

The connection between the thermal and non-thermal properties in galaxy clusters hosting radio halos seems fairly well established. However, a comprehensive analysis of such a connection has only been done for integrated quantities (e.g. LX − Pradio relation). In recent years, new-generation radio telescopes have enabled the …

2024 Astronomy and Astrophysics
XMM-Newton 7
VaTEST III: Validation of eight potential super-earths from TESS data
DOI: 10.1017/pasa.2024.29 Bibcode: 2024PASA...41...30M

Barclay, Thomas; Tan, Thiam-Guan; Schlieder, Joshua E. +39 more

NASA's all-sky survey mission, the Transiting Exoplanet Survey Satellite (TESS), is specifically engineered to detect exoplanets that transit bright stars. Thus far, TESS has successfully identified approximately 400 transiting exoplanets, in addition to roughly 6 000 candidate exoplanets pending confirmation. In this study, we present the results…

2024 Publications of the Astronomical Society of Australia
Gaia JWST 7
The Massive and Distant Clusters of WISE Survey 2: Equatorial First Data Release
DOI: 10.3847/1538-4357/ad3c44 Bibcode: 2024ApJ...967..123T

Connor, Thomas; Gonzalez, Anthony H.; Stanford, S. A. +7 more

The Massive and Distant Clusters of WISE Survey 2 (MaDCoWS2) is a new survey designed as the successor of the original MaDCoWS survey. MaDCoWS2 improves upon its predecessor by using deeper optical and infrared data and a more powerful detection algorithm (PZWav). As input to the search, we use grz photometry from the DECam Legacy Survey (DECaLS) …

2024 The Astrophysical Journal
Gaia 7