Search Publications

Black Hole Scaling Relations in the Dwarf-galaxy Regime with Gaia-Sausage/Enceladus and ωCentauri
DOI: 10.3847/2041-8213/ad9384 Bibcode: 2024ApJ...977L...2L

Limberg, Guilherme

The discovery of fast moving stars in Milky Way's most massive globular cluster, ωCentauri (ωCen), has provided strong evidence for an intermediate-mass black hole (IMBH). However, ωCen is known to be the stripped nuclear star cluster (NSC) of an ancient, now-destroyed, dwarf galaxy. The best candidate to be the original host progenitor of ωCen is…

2024 The Astrophysical Journal
Gaia 3
Resolved UV and Optical Color Gradients Reveal Environmental Influence on Galaxy Evolution at Redshift z ∼ 1.6
DOI: 10.3847/1538-4357/ad7798 Bibcode: 2024ApJ...975..144C

Cooper, M. C.; van Kampen, E.; Demarco, R. +13 more

The changes in colors across a galaxy are intimately connected to the galaxy's formation, growth, quenching history, and dust content. A particularly important epoch in the growth of galaxies is near z ∼ 2, often referred to as "cosmic noon," where galaxies on average reach the peak of their star formation. We study a population of 125 cluster gal…

2024 The Astrophysical Journal
eHST 3
Determining the Extents, Geometries, and Kinematics of Narrow-line Region Outflows in Nearby Seyfert Galaxies
DOI: 10.3847/1538-4357/ad71c3 Bibcode: 2024ApJ...975..129P

Rafelski, Marc; Fischer, Travis C.; Crenshaw, D. Michael +5 more

Outflowing gas from supermassive black holes in the centers of active galaxies has been postulated as a major contributor to galactic evolution. To explore the interaction between narrow-line region (NLR) outflows and their host galaxies, we use Hubble Space Telescope (HST) Space Telescope Imaging Spectrograph (STIS) spectra and Wide Field Camera …

2024 The Astrophysical Journal
eHST 3
Birds of a Feather: Resolving Stellar Mass Assembly with JWST/NIRCam in a Pair of Kindred z ∼ 2 Dusty Star-forming Galaxies Lensed by the PLCK G165.7+67.0 Cluster
DOI: 10.3847/1538-4357/ad5d59 Bibcode: 2024ApJ...973...25K

Grogin, Norman A.; Holwerda, Benne W.; Koekemoer, Anton M. +38 more

We present a new parametric lens model for the G165.7+67.0 galaxy cluster, which was discovered with Planck through its bright submillimeter flux, originating from a pair of extraordinary dusty star-forming galaxies (DSFGs) at z ≈ 2.2. Using JWST and interferometric mm/radio observations, we characterize the intrinsic physical properties of the DS…

2024 The Astrophysical Journal
Herschel JWST 3
Sun-as-a-star Observations of Obscuration Dimmings Caused by Filament Eruptions
DOI: 10.3847/1538-4357/ad500b Bibcode: 2024ApJ...970...60X

Veronig, Astrid M.; Dissauer, Karin; Tian, Hui +1 more

Filament eruptions often lead to coronal mass ejections (CMEs) on the Sun and are one of the most energetic eruptive phenomena in the atmospheres of other late-type stars. However, the detection of filament eruptions and CMEs on stars beyond the solar system is challenging. Here, we present six filament eruption cases on the Sun and show that fila…

2024 The Astrophysical Journal
SOHO 3
Flux Contribution and Geometry of Charge Exchange Emission in the Starburst Galaxy M82
DOI: 10.3847/1538-4357/ad1d63 Bibcode: 2024ApJ...963..147O

Foster, Adam R.; Smith, Randall K.; Okon, Hiromichi +1 more

Recent X-ray studies of starburst galaxies have found that charge exchange (CX) commonly occurs between outflowing hot plasma and cold gas, possibly from swept-up clouds. However, the total CX flux and the regions where CX occurs have been poorly understood. We present an analysis of XMM-Newton observations of M82, a prototype starburst galaxy, ai…

2024 The Astrophysical Journal
XMM-Newton eHST 3
X-Ray Variability in the Symbiotic Binary RT Cru: Principal Component Analysis
DOI: 10.3847/1538-4357/ad5cf6 Bibcode: 2024ApJ...972..109D

Luna, G. J. M.; Drake, J. J.; Danehkar, A.

Hard X-ray-emitting (δ-type) symbiotic binaries, which exhibit a strong hard X-ray excess, have posed a challenge to our understanding of accretion physics in degenerate dwarfs. RT Cru, which is a member of the δ-type symbiotics, shows stochastic X-ray variability. Timing analyses of X-ray observations from XMM-Newton and NuSTAR, which we consider…

2024 The Astrophysical Journal
XMM-Newton 3
"Beads-on-a-string" Star Formation Tied to One of the Most Powerful Active Galactic Nucleus Outbursts Observed in a Cool-core Galaxy Cluster
DOI: 10.3847/1538-4357/ad1101 Bibcode: 2024ApJ...963....1O

Baum, Stefi A.; O'Dea, Christopher P.; Vaddi, Sravani +19 more

With two central galaxies engaged in a major merger and a remarkable chain of 19 young stellar superclusters wound around them in projection, the galaxy cluster SDSS J1531+3414 (z = 0.335) offers an excellent laboratory to study the interplay between mergers, active galactic nucleus (AGN) feedback, and star formation. New Chandra X-ray imaging rev…

2024 The Astrophysical Journal
eHST 3
Toward Unveiling Cosmic Reionization: The Ionizing Photon Production Efficiency (ξ ion) of Low-mass Hα Emitters at z ∼ 2.3
DOI: 10.3847/1538-4357/ad4033 Bibcode: 2024ApJ...968...32C

Nakajima, Kimihiko; Spitler, Lee; Motohara, Kentaro +2 more

We investigate the galaxy properties of ∼400 low-mass (<109 M ) Hα emitters (HAEs) at z ∼ 2.3 in the ZFOURGE survey. The selection of these HAEs is based on the excess in the observed K s broadband flux compared to the stellar continuum estimated from the best-fit spectral energy distribution. These low-mass …

2024 The Astrophysical Journal
eHST 3
JADES Ultrared Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations
DOI: 10.3847/1538-4357/ad64c2 Bibcode: 2024ApJ...974...48G

Bunker, Andrew J.; Maiolino, Roberto; Willott, Chris +20 more

One of the more surprising findings after the first year of JWST observations is the large number of spatially extended galaxies (ultrared flattened objects, or UFOs) among the optically faint galaxy (OFG) population otherwise thought to be compact. Leveraging the depth and survey area of the JWST Advanced Deep Extragalactic Survey, we extend obse…

2024 The Astrophysical Journal
Herschel JWST 3