Search Publications

Dynamical Histories of the Crater II and Hercules Dwarf Galaxies
DOI: 10.3847/1538-4357/ab3658 Bibcode: 2019ApJ...883...11F

Simon, Joshua D.; Fu, Sal Wanying; Alarcón Jara, Alex G.

We investigate the possibility that the dwarf galaxies Crater II and Hercules have previously been tidally stripped by the Milky Way. We present Magellan/IMACS spectra of candidate member stars in both objects. We identify 37 members of Crater II, 25 of which have velocity measurements in the literature, and we classify three stars within that sub…

2019 The Astrophysical Journal
Gaia 40
Extended Main-sequence Turnoffs in the Double Cluster h and χ Persei: The Complex Role of Stellar Rotation
DOI: 10.3847/1538-4357/ab15d2 Bibcode: 2019ApJ...876...65L

Milone, Antonino P.; Cordoni, Giacomo; Deng, Licai +4 more

Using Gaia Data Release 2 photometry, we report the detection of extended main-sequence turnoff (eMSTO) regions in the color-magnitude diagrams (CMDs) of the ∼14 Myr old double clusters h and χ Persei (NGC 869 and NGC 884). We find that stars with masses below ∼1.3 M in both h and χ Persei populate narrow main sequences (MSs), while m…

2019 The Astrophysical Journal
Gaia 40
The Resolved Distributions of Dust Mass and Temperature in Local Group Galaxies
DOI: 10.3847/1538-4357/ab05d3 Bibcode: 2019ApJ...874..141U

Sandstrom, Karin M.; Leroy, Adam K.; Chiang, I-Da +2 more

We utilize archival far-infrared maps from the Herschel Space Observatory in four Local Group galaxies (Small and Large Magellanic Clouds (SMC and LMC), M31, and M33). We model their spectral energy distribution from 100 to 500 µm using a single-temperature modified blackbody emission with a fixed emissivity index of β = 1.8. From the best-f…

2019 The Astrophysical Journal
Herschel eHST 40
UVIT Open Cluster Study. I. Detection of a White Dwarf Companion to a Blue Straggler in M67: Evidence of Formation through Mass Transfer
DOI: 10.3847/1538-4357/ab31a8 Bibcode: 2019ApJ...882...43S

Jadhav, Vikrant V.; Puzia, Thomas H.; Simunovic, Mirko +7 more

The old open cluster M67, populated with blue straggler stars (BSSs), is a well-known test bed to study the BSS formation pathways. Here, we report the first direct detection of a white dwarf (WD) companion to a BSS in M67, using far-UV images from the Ultra-Violet Imaging telescope on ASTROSAT. Near-simultaneous observations in three far-UV bands…

2019 The Astrophysical Journal
Gaia IUE 40
Space Telescope and Optical Reverberation Mapping Project. VIII. Time Variability of Emission and Absorption in NGC 5548 Based on Modeling the Ultraviolet Spectrum
DOI: 10.3847/1538-4357/ab3049 Bibcode: 2019ApJ...881..153K

Im, M.; Malkan, M. A.; Geier, S. +164 more

We model the ultraviolet spectra of the Seyfert 1 galaxy NGC 5548 obtained with the Hubble Space Telescope during the 6 month reverberation mapping campaign in 2014. Our model of the emission from NGC 5548 corrects for overlying absorption and deblends the individual emission lines. Using the modeled spectra, we measure the response to continuum v…

2019 The Astrophysical Journal
XMM-Newton eHST 40
Buried Black Hole Growth in IR-selected Mergers: New Results from Chandra
DOI: 10.3847/1538-4357/ab07bc Bibcode: 2019ApJ...875..117P

Ellison, Sara L.; Ricci, Claudio; Blecha, Laura +8 more

Observations and theoretical simulations suggest that a significant fraction of merger-triggered accretion onto supermassive black holes is highly obscured, particularly in late-stage galaxy mergers, when the black hole is expected to grow most rapidly. Starting with the Wide-Field Infrared Survey Explorer all-sky survey, we identified a populatio…

2019 The Astrophysical Journal
XMM-Newton 40
Comparing the Quenching Times of Faint M31 and Milky Way Satellite Galaxies
DOI: 10.3847/2041-8213/ab4b52 Bibcode: 2019ApJ...885L...8W

Lewis, Geraint F.; Dolphin, Andrew E.; Skillman, Evan D. +8 more

We present the star formation histories (SFHs) of 20 faint M31 satellites (-12 ≲ M V ≲ -6) that were measured by modeling sub-horizontal branch depth color-magnitude diagrams constructed from Hubble Space Telescope (HST) imaging. Reinforcing previous results, we find that virtually all galaxies quenched between 3 and 9 Gyr ago, indepe…

2019 The Astrophysical Journal
eHST 40
Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z = 1.522
DOI: 10.3847/2041-8213/ab0c9c Bibcode: 2019ApJ...873L..19B

Franx, Marijn; Bezanson, Rachel; Weiner, Benjamin +4 more

One of the greatest challenges to theoretical models of massive galaxy formation is the regulation of star formation at early times. The relative roles of molecular gas expulsion, depletion, and stabilization are uncertain as direct observational constraints of the gas reservoirs in quenched or quenching galaxies at high redshift are scant. We pre…

2019 The Astrophysical Journal
eHST 39
The TRGB Distance to the Second Galaxy “Missing Dark Matter”: Evidence for Two Groups of Galaxies at 13.5 and 19 Mpc in the Line of Sight of NGC 1052
DOI: 10.3847/2041-8213/ab2fd2 Bibcode: 2019ApJ...880L..11M

Trujillo, Ignacio; Monelli, Matteo

A second galaxy “missing dark matter” (NGC 1052-DF4) has been reported recently. Here we show, using the location of the tip of the red giant branch (TRGB), that the distance to this galaxy is 14.2 ± 0.7 Mpc. This locates the galaxy 6 Mpc closer than previously determined. We also analyze the distances to the brightest galaxies in the field of vie…

2019 The Astrophysical Journal
eHST 39
RELICS: Strong Lensing Analysis of MACS J0417.5-1154 and Predictions for Observing the Magnified High-redshift Universe with JWST
DOI: 10.3847/1538-4357/ab042b Bibcode: 2019ApJ...873...96M

Ouchi, Masami; Mahler, Guillaume; Frye, Brenda L. +37 more

Strong gravitational lensing by clusters of galaxies probes the mass distribution at the core of each cluster and magnifies the universe behind it. MACS J0417.5-1154 at z = 0.443 is one of the most massive clusters known based on weak lensing, X-ray, and Sunyaev-Zel’dovich analyses. Here we compute a strong lens model of MACS J0417 based on Hubble…

2019 The Astrophysical Journal
eHST 39