Search Publications

The Evolution of Stellar X-Ray Activity and Angular Momentum as Seen by eROSITA, TESS, and Gaia
DOI: 10.3847/2041-8213/ad4c64 Bibcode: 2024ApJ...967L..36S

Stassun, Keivan G.; Kounkel, Marina

We have assembled a sample of ∼8200 stars with spectral types F5V–M5V, all having directly measured X-ray luminosities from eROSITA and rotation periods from TESS and having empirically estimated ages via their membership in stellar clusters and groups identified in Gaia astrometry (ages 3–500 Myr). This is the largest such study sample yet assemb…

2024 The Astrophysical Journal
Gaia 1
Thermal Evolution of an Active Region Through Quiet and Flaring Phases as Observed by NuSTAR, XRT, and AIA
DOI: 10.3847/1538-4357/ad37f7 Bibcode: 2024ApJ...966..197D

Reeves, Katharine K.; Grefenstette, Brian W.; Shih, Albert Y. +6 more

Solar active regions (ARs) contain a broad range of temperatures, with the thermal plasma distribution often observed to peak in the few millions of kelvin. Differential emission measure (DEM) analysis can allow instruments with diverse temperature responses to be used in concert to estimate this distribution. Nuclear Spectroscopic Telescope ARray…

2024 The Astrophysical Journal
Hinode 1
Constraining the Progenitor of the Nearby Type II-P SN 2024ggi with Environmental Analysis
DOI: 10.3847/2041-8213/ad99da Bibcode: 2024ApJ...977L..50H

Niu, Zexi; Sun, Ning-Chen; Liu, Jifeng +3 more

The progenitors of Type II-P supernovae (SN) have been confirmed to be red supergiants. However, the upper mass limit of the directly probed progenitors is much lower than that predicted by current theories, and the accurate determination of the progenitor masses is key to understand the final fate of massive stars. Located at a distance of only 6…

2024 The Astrophysical Journal
eHST 1
Active Galactic Nuclei in the Green Valley at z ∼ 0.7
DOI: 10.3847/1538-4357/ad74f1 Bibcode: 2024ApJ...974..305W

Ji, Zhiyuan; Rieke, Marcia; Williams, Christina C. +5 more

We present near-infrared (NIR) spectroscopy using the MMT and Magellan infrared spectrograph for a sample of 29 massive galaxies ( logM*/M

2024 The Astrophysical Journal
eHST 1
An analysis of spectroscopic, seismological, astrometric, and photometric masses of pulsating white dwarf stars
DOI: 10.1051/0004-6361/202450582 Bibcode: 2024A&A...691A.194C

Kepler, S. O.; Córsico, Alejandro H.; Uzundag, Murat +3 more

Context. A central challenge in the field of stellar astrophysics lies in accurately determining the mass of stars, particularly when dealing with isolated ones. However, for pulsating white dwarf stars, the task becomes more tractable due to the availability of multiple approaches such as spectroscopy, asteroseismology, astrometry, and photometry…

2024 Astronomy and Astrophysics
Gaia 1
A Statistical Study of Magnetic Flux Emergence in Solar Active Regions Prior to Strongest Flares
DOI: 10.1088/1674-4527/ad2e4d Bibcode: 2024RAA....24d5014K

Abramenko, Valentina I.; Kutsenko, Alexander S.; Plotnikov, Andrei A.

Using the data on magnetic field maps and continuum intensity for Solar Cycles 23 and 24, we explored 100 active regions (ARs) that produced M5.0 or stronger flares. We focus on the presence/absence of the emergence of magnetic flux in these ARs 2–3 days before the strong flare onset. We found that 29 ARs in the sample emerged monotonically amidst…

2024 Research in Astronomy and Astrophysics
SOHO 1
TESSILATOR: a one-stop shop for measuring TESS rotation periods
DOI: 10.1093/mnras/stae1850 Bibcode: 2024MNRAS.533.2162B

Günther, H. M.; Binks, A. S.

We present a software package designed to produce photometric light curves and measure rotation periods from full-frame images taken by the Transiting Exoplanet Survey Satellite (TESS), which we name 'TESSILATOR'. TESSILATOR is the only publicly available code that will run a full light curve and rotation period ($P_{\rm rot}$) analysis based on j…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
Ongoing and Fossil Large-scale Outflows Detected in a High-redshift Radio Galaxy: [C II] Observations of TN J0924-2201 at z = 5.174
DOI: 10.3847/1538-4357/ad5be5 Bibcode: 2024ApJ...972..111L

Imanishi, Masatoshi; Kohno, Kotaro; Schramm, Malte +13 more

We present Atacama Large Millimeter/submillimeter Array observations of the [C II] 158 µm line and the underlying continuum emission of TN J0924‑2201, which is one of the most distant known radio galaxies at z > 5. The [C II] line and 1 mm continuum emission are detected at the host galaxy. The systemic redshift derived from the [C II] li…

2024 The Astrophysical Journal
eHST 1
Europa's H2O2: Temperature Insensitivity and a Correlation with CO2
DOI: 10.3847/PSJ/ad7468 Bibcode: 2024PSJ.....5..220W

Brown, Michael E.; de Kleer, Katherine; Trumbo, Samantha K. +1 more

H2O2 is part of Europa's water-ice radiolytic cycle and a potential source of oxidants to Europa's subsurface ocean. However, factors controlling the concentration of this critical surface species remain unclear. Though laboratory experiments suggest that Europa's H2O2 should be concentrated in the colde…

2024 The Planetary Science Journal
JWST 1
A model of light pseudoscalar dark matter
DOI: 10.1016/j.nuclphysb.2024.116721 Bibcode: 2024NuPhB100816721C

Chakdar, Shreyashi; Ghosh, Dilip Kumar; Hung, P. Q. +2 more

The EW-νR model was constructed in order to provide a seesaw scenario operating at the Electroweak scale Λ

2024 Nuclear Physics B
INTEGRAL 1