Search Publications

Detection of a Multiphase Intragroup Medium: Results from the COS-IGrM Survey
DOI: 10.3847/1538-4357/ac283c Bibcode: 2021ApJ...923..189M

Heckman, Timothy; Tumlinson, Jason; Borthakur, Sanchayeeta +3 more

We present the results of the Cosmic Origins Spectrograph-Intragroup Medium (COS-IGrM) Survey that used the COS on the Hubble Space Telescope to observe a sample of 18 UV bright quasars, each probing the IGrM of a galaxy group. We detect Lyα, C II, N V, Si II, Si III, and O VI in multiple sightlines. The highest ionization species detected in our …

2021 The Astrophysical Journal
eHST 10
In the Trenches of the Solar-stellar Connection. IV. Solar Full-disk Scans of C II, Si IV, and Mg II by the Interface Region Imaging Spectrograph
DOI: 10.3847/1538-4357/abfa92 Bibcode: 2021ApJ...916...36A

Testa, Paola; De Pontieu, Bart; Ayres, Thomas

About once a month, the Interface Region Imaging Spectrograph conducts day-long raster scans of the full Sun in three ultraviolet spectral channels. These full-disk mosaics are valuable in the solar context, but provide a unique connection to the distant, unresolved stars. Here, 10 deep-exposure scans (4-8 s per slit step), collected during the pe…

2021 The Astrophysical Journal
IRIS eHST 10
In the Trenches of the Solar-Stellar Connection. III. The HST/COS Ecliptic-poles Stellar Survey (EclipSS)
DOI: 10.3847/1538-4357/abd7a2 Bibcode: 2021ApJ...910...71A

Ayres, Thomas R.

The Ecliptic-poles Stellar Survey (EclipSS) collected far-ultraviolet (FUV: 1160-1420 Å) spectra of 49 nearby (d ≲ 100 pc) F3-K3 main-sequence stars, located at high ecliptic latitudes (north and south), using the Cosmic Origins Spectrograph of the Hubble Space Telescope. The ecliptic poles receive higher exposures from scanning missions like the …

2021 The Astrophysical Journal
Gaia IRIS eHST 10
A Hard Look at Relativistic Reverberation in MCG-5-23-16 and SWIFT J2127.4+5654: Testing the Lamppost Model
DOI: 10.3847/1538-4357/abebd9 Bibcode: 2021ApJ...912...42Z

Miller, J. M.; Zoghbi, A.; Cackett, E.

X-ray reverberation mapping has emerged as a new tool to probe accretion in active galactic nuclei (AGN), providing a potentially powerful probe of accretion at the black hole scale. The lags, along with relativistic spectral signatures are often interpreted in light of the lamppost model. Focusing specifically on testing the prediction of the rel…

2021 The Astrophysical Journal
XMM-Newton 10
The Merger Dynamics of the Galaxy Cluster A1775: New Insights from Chandra and XMM-Newton for a Cluster Simultaneously Hosting a Wide-angle Tail and a Narrow-angle Tail Radio Source
DOI: 10.3847/1538-4357/abf09e Bibcode: 2021ApJ...913....8H

Hu, Dan; Xu, Haiguang; Zhu, Zhenghao +13 more

We present a new study of the merger dynamics of A1775 by analyzing the high-quality Chandra and XMM-Newton archival data. We confirm/identify an arc-shaped edge (i.e., the head) at ∼48 kpc west of the X-ray peak, a split cold gas tail that extends eastward to ∼163 kpc, and a plume of spiral-like X-ray excess (within about 81-324 kpc northeast of …

2021 The Astrophysical Journal
XMM-Newton 10
Multiple Populations in Low-mass Globular Clusters: Palomar 13
DOI: 10.3847/1538-4357/abd557 Bibcode: 2021ApJ...908..220T

Carballo-Bello, Julio A.; Li, Chengyuan; Cabrera-Lavers, Antonio +7 more

Since the discovery of chemically peculiar stars in globular clusters in the last century, the study of multiple populations has become increasingly important, given that chemical inhomogeneity is found in almost all globular clusters. Despite various proposed theories attempting to explain this phenomenon, fitting all the observational evidence i…

2021 The Astrophysical Journal
Gaia 10
Chemical Analysis of Two Extremely Metal-poor Stars HE 2148-2039 and HE 2155-2043
DOI: 10.3847/1538-4357/abec45 Bibcode: 2021ApJ...912...74P

Goswami, Aruna; Purandardas, Meenakshi

We present elemental abundance results for HE 2148-2039 and HE 2155-2043 based on a detailed high-resolution spectroscopic analysis. The high-resolution Subaru/High Dispersion Spectrograph (HDS) spectra used for our analysis have a resolution of R ∼ 60,000. Although limited information based on photometry and low-resolution spectroscopy is availab…

2021 The Astrophysical Journal
Gaia 10
Cooling Models for the Most Massive White Dwarfs
DOI: 10.3847/1538-4357/ac0336 Bibcode: 2021ApJ...916..119S

Schwab, Josiah

We present a set of ultramassive white dwarf models, focused on masses above 1.3 M. Given the uncertainties about the formation and compositions of such objects, we construct parameterized model sequences, guided by evolutionary calculations including both single star and double white dwarf merger formation channels. We demonstrate tha…

2021 The Astrophysical Journal
Gaia 10
The ACTIONFINDER: An Unsupervised Deep Learning Algorithm for Calculating Actions and the Acceleration Field from a Set of Orbit Segments
DOI: 10.3847/1538-4357/abfda9 Bibcode: 2021ApJ...915....5I

Famaey, Benoit; Ibata, Rodrigo; Monari, Giacomo +1 more

We introduce the ACTIONFINDER, a deep learning algorithm designed to transform a sample of phase-space measurements along orbits in a static potential into action and angle coordinates. The algorithm finds the mapping from positions and velocities to actions and angles in an unsupervised way, by using the fact that points along the same orbit have…

2021 The Astrophysical Journal
Gaia 10
The Mass and Age Distribution of Halo White Dwarfs in the Canada-France Imaging Survey
DOI: 10.3847/1538-4357/abf2b2 Bibcode: 2021ApJ...913...30F

Gwyn, Stephen D. J.; McConnachie, Alan W.; Cuillandre, Jean-Charles +6 more

We present optical spectroscopy for 18 halo white dwarfs identified using photometry from the Canada-France Imaging Survey and Pan-STARRS1 DR1 3π survey combined with astrometry from Gaia DR2. The sample contains 13 DA, 1 DZ, 2 DC, and 2 potentially exotic types of white dwarf. We fit both the spectrum and the spectral energy distribution in order…

2021 The Astrophysical Journal
Gaia 10