Search Publications

Atmospheric Characterization of Hot Jupiter CoRoT-1 b Using the Wide Field Camera 3 on the Hubble Space Telescope
DOI: 10.3847/1538-3881/ac6cdb Bibcode: 2022AJ....164...19G

Deming, Drake; Zhou, Yifan; Schlawin, Everett +3 more

Exoplanet CoRoT-1 b is intriguing because we predict it to be a transitional planet between hot Jupiters (equilibrium temperatures ~1500 K) and ultrahot Jupiters (equilibrium temperatures >2000 K). In 2012, observations of CoRoT-1 b included one primary transit and three secondary eclipses with the Hubble Space Telescope (HST) Wide Field Camera…

2022 The Astronomical Journal
eHST 12
A 6D view of stellar shells
DOI: 10.1093/mnras/stab3361 Bibcode: 2022MNRAS.510..230D

Evans, N. W.; Vasiliev, E.; Dong-Páez, C. A.

Stellar shells are low surface brightness features, created during nearly head-on galaxy mergers from the debris of the tidally disrupted satellite. Here, we investigate the formation and evolution mechanism of shells in six dimensions (3D positions and velocities). We propose a new description in action-angle coordinates which condenses the seemi…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 12
Manifestation of Gravitational Settling in Coronal Mass Ejections Measured in the Heliosphere
DOI: 10.3847/1538-4357/ac8873 Bibcode: 2022ApJ...936...83R

Reeves, Katharine K.; Landi, Enrico; Raymond, John C. +4 more

Elemental composition in the solar wind reflects the fractionation processes at the Sun. In coronal mass ejections (CMEs) measured in the heliosphere, the elemental composition can vary between plasma of high and low ionization states as indicated by the average Fe charge state, <QFe>. It is found that CMEs with higher ionized pla…

2022 The Astrophysical Journal
SOHO 12
CAPOS: The bulge Cluster APOgee Survey. III. Spectroscopic tomography of Tonantzintla 2
DOI: 10.1051/0004-6361/202141742 Bibcode: 2022A&A...658A.116F

Cohen, Roger E.; Beers, Timothy C.; Minniti, Dante +10 more

We performed the first detailed spectral analysis of red giant members of the relatively high-metallicity globular cluster (GC) Tononzintla 2 (Ton 2) using high-resolution near-infrared spectra collected with the Apache Point Observatory Galactic Evolution Experiment II survey (APOGEE-2), obtained as part of the bulge Cluster APOgee Survey. We inv…

2022 Astronomy and Astrophysics
Gaia 12
Differences in star formation activity between tidally triggered and isolated bars: a case study of NGC 4303 and NGC 3627
DOI: 10.1093/mnras/stab3330 Bibcode: 2022MNRAS.510.3899I

Okamoto, Takashi; Pettitt, Alex R.; Iles, Elizabeth J.

Galactic bars are important drivers of galactic evolution, and yet how they impact the interstellar medium and correspondingly star formation, remains unclear. We present simulation results for two barred galaxies with different formation mechanisms, bars formed in isolation or via a tidal interaction, to consider the spatially and temporally vary…

2022 Monthly Notices of the Royal Astronomical Society
eHST 12
A Roche lobe-filling hot subdwarf and white dwarf binary: possible detection of an ejected common envelope
DOI: 10.1093/mnras/stac1768 Bibcode: 2022MNRAS.515.3370L

Wang, Luqian; Han, Zhanwen; Chen, Xuefei +12 more

Binaries consisting of a hot subdwarf star and an accreting white dwarf (WD) are sources of gravitational wave radiation at low frequencies and possible progenitors of Type Ia supernovae if the WD mass is large enough. Here, we report the discovery of the third binary known of this kind: It consists of a hot subdwarf O (sdO) star and a WD with an …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 12
A chemical map of the outbursting V883 Ori system: vertical and radial structures
DOI: 10.1093/mnras/stac1879 Bibcode: 2022MNRAS.515.2646R

Kastner, J. H.; Williams, J. P.; Cieza, L. +3 more

We present the first results of a pilot program to conduct an Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 (211-275 GHz) spectral line study of young stellar objects (YSOs) that are undergoing rapid accretion episodes, i.e. FU Ori objects (FUors). Here, we report on molecular emission line observations of the FUor system, V883 Ori. I…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 12
Dynamical Friction in Globular Cluster-rich Ultra-diffuse Galaxies: The Case of NGC5846-UDG1
DOI: 10.3847/2041-8213/ac70df Bibcode: 2022ApJ...932L..10B

Danieli, Shany; Bar, Nitsan; Blum, Kfir

Ultra-diffuse galaxies that contain a large sample of globular clusters (GCs) offer an opportunity to test the predictions of galactic dynamics theory. NGC5846-UDG1 is an excellent example, with a high-quality sample of dozens of GC candidates. We show that the observed distribution of GCs in NGC5846-UDG1 is suggestive of mass segregation induced …

2022 The Astrophysical Journal
eHST 12
Is [Y/Mg] a Reliable Age Diagnostic for FGK Stars?
DOI: 10.3847/1538-4357/ac8746 Bibcode: 2022ApJ...936..100B

van Saders, Jennifer L.; Huber, Daniel; Claytor, Zachary R. +3 more

Current spectroscopic surveys are producing large catalogs of chemical abundances for stars of all types. The yttrium-to-magnesium ratio, [Y/Mg], has emerged as a candidate age indicator for solar twins in the local stellar neighborhood. However, it is unclear whether it is a viable age diagnostic for more diverse stellar types, so we investigate …

2022 The Astrophysical Journal
Gaia 12
Searching for a Hypervelocity White Dwarf SN Ia Companion: A Proper-motion Survey of SN 1006
DOI: 10.3847/2041-8213/ac7950 Bibcode: 2022ApJ...933L..31S

Lu, Jessica R.; Rest, Armin; Zenteno, Alfredo +7 more

Type Ia supernovae (SNe Ia) are securely understood to come from the thermonuclear explosion of a white dwarf as a result of binary interaction, but the nature of that binary interaction and the secondary object is uncertain. Recently, a double white dwarf model known as the dynamically driven double-degenerate double-detonation (D6) model has bec…

2022 The Astrophysical Journal
Gaia 12