Search Publications

Modeling the High-energy Ionizing Output from Simple Stellar and X-Ray Binary Populations
DOI: 10.3847/1538-4357/ad0a6a Bibcode: 2024ApJ...960...13G

Johnson, Benjamin D.; Tzanavaris, Panayiotis; Jaskot, Anne +9 more

We present a methodology for modeling the joint ionizing impact due to a "simple X-ray population" (SXP) and its corresponding simple stellar population (SSP), where "simple" refers to a single age and metallicity population. We construct composite spectral energy distributions (SEDs) including contributions from ultraluminous X-ray sources and st…

2024 The Astrophysical Journal
eHST 16
JWST Imaging of Edge-on Protoplanetary Disks. II. Appearance of Edge-on Disks with a Tilted Inner Region: Case Study of IRAS04302+2247
DOI: 10.3847/1538-4357/ad0c4b Bibcode: 2024ApJ...961...95V

Duchêne, Gaspard; Wolff, Schuyler G.; Perrin, Marshall D. +6 more

We present James Webb Space Telescope imaging from 2 to 21 µm of the edge-on protoplanetary disk around the embedded young star IRAS04302+2247. The structure of the source shows two reflection nebulae separated by a dark lane. The source extent is dominated by the extended filamentary envelope at ~4.4 µm and shorter wavelengths, transi…

2024 The Astrophysical Journal
Gaia eHST JWST 16
Kinematics and dynamics of the Galactic bar revealed by Gaia long-period variables
DOI: 10.1093/mnras/stae2023 Bibcode: 2024MNRAS.533.3395Z

Belokurov, Vasily; Zhang, Hanyuan; Evans, N. Wyn +2 more

We use low-amplitude long period variable (LA-LPV) candidates in Gaia DR3 to trace the kinematics and dynamics of the Milky Way bar. LA-LPVs, like other LPVs, are intrinsically bright and follow a tight period-luminosity relation, but unlike e.g. Mira variables, their radial velocity measurements are reliable due to their smaller pulsation amplitu…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 16
Galaxy assembly revealed by globular clusters
DOI: 10.33232/001c.116169 Bibcode: 2024OJAp....7E..23C

Chen, Yingtian; Gnedin, Oleg Y.

Many observable properties of globular clusters (GCs) provide valuable insights for unveiling the hierarchical assembly of their host galaxy. For the Milky Way (MW) in particular, GCs from different accreted satellite galaxies show distinct chemical, spatial, kinematic, and age distributions. Here we examine such clustering features for model GC p…

2024 The Open Journal of Astrophysics
Gaia 15
A case for a binary black hole system revealed via quasi-periodic outflows
DOI: 10.1126/sciadv.adj8898 Bibcode: 2024SciA...10J8898P

Steiner, James F.; Holoien, Thomas W. -S.; Daylan, Tansu +33 more

Binaries containing a compact object orbiting a supermassive black hole are thought to be precursors of gravitational wave events, but their identification has been extremely challenging. Here, we report quasi-periodic variability in x-ray absorption, which we interpret as quasi-periodic outflows (QPOuts) from a previously low-luminosity active ga…

2024 Science Advances
XMM-Newton 15
Probing the early Milky Way with GHOST spectra of an extremely metal-poor star in the Galactic disc
DOI: 10.1093/mnras/stad3673 Bibcode: 2024MNRAS.527.7810D

Simpson, Chris; Placco, Vinicius M.; Hayes, Christian R. +31 more

Pristine_183.6849 + 04.8619 (P1836849) is an extremely metal-poor ([Fe/H] = -3.3 ± 0.1) star on a prograde orbit confined to the Galactic disc. Such stars are rare and may have their origins in protogalactic fragments that formed the early Milky Way, in low-mass satellites accreted later, or forming in situ in the Galactic plane. Here, we present …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 15
UVCANDELS: The Role of Dust on the Stellar Mass–Size Relation of Disk Galaxies at 0.5 ≤ z ≤ 3.0
DOI: 10.3847/1538-4357/ad4ede Bibcode: 2024ApJ...970..188N

Grogin, Norman A.; Koekemoer, Anton M.; Lucas, Ray A. +30 more

We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest-frame far-UV for ∼16,000 disk-like galaxies over 0.5 ≤ z ≤ 3. We compare these results to rest-frame optical sizes that we measure in a self-consistent way and find that the stellar mass–si…

2024 The Astrophysical Journal
eHST 15
JWST lensed quasar dark matter survey - I. Description and first results
DOI: 10.1093/mnras/stae499 Bibcode: 2024MNRAS.530.2960N

Djorgovski, S. G.; Stern, D.; Treu, T. +18 more

The flux ratios of gravitationally lensed quasars provide a powerful probe of the nature of dark matter. Importantly, these ratios are sensitive to small-scale structure, irrespective of the presence of baryons. This sensitivity may allow us to study the halo mass function even below the scales where galaxies form observable stars. For accurate me…

2024 Monthly Notices of the Royal Astronomical Society
eHST JWST 15
JWST Spectroscopy of SN H0pe: Classification and Time Delays of a Triply Imaged Type Ia Supernova at z = 1.78
DOI: 10.3847/1538-4357/ad50a5 Bibcode: 2024ApJ...970..102C

Grogin, Norman A.; Koekemoer, Anton M.; Frye, Brenda L. +19 more

SN H0pe is a triply imaged supernova (SN) at redshift z = 1.78 discovered using the James Webb Space Telescope. In order to classify the SN spectroscopically and measure the relative time delays of its three images (designated A, B, and C), we acquired NIRSpec follow-up spectroscopy spanning 0.6–5 µm. From the high signal-to-noise spectra of…

2024 The Astrophysical Journal
JWST 15
The Fraction of Dust Mass in the Form of Polycyclic Aromatic Hydrocarbons on 10–50 pc Scales in Nearby Galaxies
DOI: 10.3847/1538-4357/ad54bd Bibcode: 2024ApJ...971..178S

Ramambason, Lise; Leroy, Adam K.; Rosolowsky, Erik +21 more

Polycyclic aromatic hydrocarbons (PAHs) are a ubiquitous component of the interstellar medium (ISM) in z ∼ 0 massive, star-forming galaxies and play key roles in ISM energy balance, chemistry, and shielding. Wide field-of-view, high-resolution mid-infrared (MIR) images from JWST provide the ability to map the fraction of dust in the form of PAHs a…

2024 The Astrophysical Journal
Herschel JWST 15