Search Publications

Spectroscopy and Photometry of the Least Massive Type II Globular Clusters: NGC 1261 and NGC 6934
DOI: 10.3847/1538-4357/ac282c Bibcode: 2021ApJ...923...22M

Da Costa, G. S.; Milone, A. P.; Cordoni, G. +10 more

Recent work has revealed two classes of globular clusters (GCs), dubbed Type I and Type II. Type II GCs are characterized by both a blue and a red red giant branch composed of stars with different metallicities, often coupled with distinct abundances in the slow neutron-capture elements (s-elements). Here we continue the chemical tagging of Type I…

2021 The Astrophysical Journal
eHST 26
Resolving the Dust-to-Metals Ratio and CO-to-H2 Conversion Factor in the Nearby Universe
DOI: 10.3847/1538-4357/abceb6 Bibcode: 2021ApJ...907...29C

Sandstrom, Karin M.; Leroy, Adam K.; Schruba, Andreas +8 more

We investigate the relationship between the dust-to-metals ratio (D/M) and the local interstellar medium environment at ∼2 kpc resolution in five nearby galaxies: IC 342, M31, M33, M101, and NGC 628. A modified blackbody model with a broken power-law emissivity is used to model the dust emission from 100 to 500 µm observed by Herschel. We ut…

2021 The Astrophysical Journal
Herschel 26
Grain Growth in Escaping Atmospheres: Implications for the Radius Inflation of Super-Puffs
DOI: 10.3847/1538-4357/ac1516 Bibcode: 2021ApJ...920..124O

Ohno, Kazumasa; Tanaka, Yuki A.

Super-puffs-low-mass exoplanets with extremely low bulk density-are attractive targets for exploring their atmospheres and formation processes. Recent studies suggested that the large radii of super-puffs may be caused by atmospheric dust entrained in the escaping atmospheres. In this study, we investigate how the dust grows in escaping atmosphere…

2021 The Astrophysical Journal
eHST 26
Head-to-Toe Measurement of El Gordo: Improved Analysis of the Galaxy Cluster ACT-CL J0102-4915 with New Wide-field Hubble Space Telescope Imaging Data
DOI: 10.3847/1538-4357/ac294f Bibcode: 2021ApJ...923..101K

Sifón, Cristóbal; Hughes, John P.; Jee, M. James +6 more

We present an improved weak-lensing (WL) study of the high-z (z = 0.87) merging galaxy cluster ACT-CL J0102-4915 ("El Gordo") based on new wide-field Hubble Space Telescope imaging data. The new imaging data cover the ~3.5 × ~3.5 Mpc region centered on the cluster and enable us to detect WL signals beyond the virial radius, which was not possible …

2021 The Astrophysical Journal
eHST 26
Revisiting Dynamical Friction: The Role of Global Modes and Local Wakes
DOI: 10.3847/1538-4357/ac0627 Bibcode: 2021ApJ...916...55T

Babul, Arif; Quinn, Thomas R.; Mayer, Lucio +4 more

The orbital decay of a perturber within a larger system plays a key role in the dynamics of many astrophysical systems-from nuclear star clusters or globular clusters in galaxies, to massive black holes in galactic nuclei, to dwarf galaxy satellites within the dark matter halos of more massive galaxies. For many decades, there have been various at…

2021 The Astrophysical Journal
Gaia 26
R-process-rich Stellar Streams in the Milky Way
DOI: 10.3847/1538-4357/abea1a Bibcode: 2021ApJ...912...52G

Roederer, Ian U.; Frebel, Anna; Ji, Alexander P. +3 more

We present high-resolution Magellan/MIKE spectra of 22 bright (9 < V < 13.5) metal-poor stars (-3.18 < [Fe/H] < -1.37) in three different stellar streams, the Helmi debris stream, the Helmi trail stream, and the ω Centauri progenitor stream. We augment our Helmi debris sample with results for 10 stars by Roederer et al. for a total of …

2021 The Astrophysical Journal
Gaia 25
ALMA Observations of the Sub-kpc Structure of the Host Galaxy of a z = 6.5 Lensed Quasar: A Rotationally Supported Hyper-Starburst System at the Epoch of Reionization
DOI: 10.3847/1538-4357/ac0af4 Bibcode: 2021ApJ...917...99Y

Fan, Xiaohui; Keeton, Charles R.; Walter, Fabian +11 more

We report Atacama Large Millimeter/Submillimeter Array (ALMA) observations of the dust continuum and [C II] emission of the host galaxy of J0439+1634, a gravitationally lensed quasar at z = 6.5. Gravitational lensing boosts the source-plane resolution to ~0"15 (~0.8 kpc). The lensing model derived from the ALMA data is consistent with the fiducial…

2021 The Astrophysical Journal
eHST 25
TESS Asteroseismology of α Mensae: Benchmark Ages for a G7 Dwarf and Its M Dwarf Companion
DOI: 10.3847/1538-4357/ac1269 Bibcode: 2021ApJ...922..229C

Butler, R. Paul; Chaplin, William J.; Stassun, Keivan G. +27 more

Asteroseismology of bright stars has become increasingly important as a method to determine the fundamental properties (in particular ages) of stars. The Kepler Space Telescope initiated a revolution by detecting oscillations in more than 500 main-sequence and subgiant stars. However, most Kepler stars are faint and therefore have limited constrai…

2021 The Astrophysical Journal
Gaia 25
Inspecting the Cepheid Distance Ladder: the Hubble Space Telescope Distance to the SN Ia Host Galaxy NGC 5584
DOI: 10.3847/1538-4357/abe7e5 Bibcode: 2021ApJ...911...12J

Mérand, Antoine; Breuval, Louise; Gieren, Wolfgang +7 more

The current tension between the direct and the early-universe measurements of the Hubble constant, H0, requires detailed scrutiny of all the data and methods used in the studies on both sides of the debate. The Cepheids in the Type Ia supernova (SN Ia) host galaxy NGC 5584 played a key role in the local measurement of H0. The…

2021 The Astrophysical Journal
Gaia eHST 25
Further Evidence for Tidal Spin-up of Hot Jupiter Host Stars
DOI: 10.3847/1538-4357/ac1429 Bibcode: 2021ApJ...919..138T

Winn, Joshua N.; Anderson, Kassandra R.; Tejada Arevalo, Roberto A.

For most hot Jupiters around main-sequence Sun-like stars, tidal torques are expected to transfer angular momentum from the planet's orbit to the star's rotation. The timescale for this process is difficult to calculate, leading to uncertainties in the history of orbital evolution of hot Jupiters. We present evidence for tidal spin-up by taking ad…

2021 The Astrophysical Journal
Gaia 25