Search Publications

The Panchromatic Hubble Andromeda Treasury. XXI. The Legacy Resolved Stellar Photometry Catalog
DOI: 10.3847/1538-4365/acea61 Bibcode: 2023ApJS..268...48W

Bell, Eric F.; Dolphin, Andrew E.; Yanchulova Merica-Jones, Petia +14 more

We present the final legacy version of stellar photometry for the Panchromatic Hubble Andromeda Treasury (PHAT) survey. We have reprocessed all of the Hubble Space Telescope Wide Field Camera 3 and Advanced Camera for Surveys near-ultraviolet (F275W, F336W), optical (F475W, F814W), and near-infrared (F110W, F160W) imaging from the PHAT survey usin…

2023 The Astrophysical Journal Supplement Series
eHST 6
Formulating Mass-loss Rates for Sun-like Stars: A Hybrid Model Approach
DOI: 10.3847/1538-4357/acfa72 Bibcode: 2023ApJ...957...71S

Toriumi, Shin; Cranmer, Steven R.; Shoda, Munehito

We observe an enhanced stellar wind mass-loss rate from low-mass stars exhibiting higher X-ray flux. This trend, however, does not align with the Sun, where no evident correlation between X-ray flux and mass-loss rate is present. To reconcile these observations, we propose a hybrid model for the stellar wind from solar-type stars, incorporating bo…

2023 The Astrophysical Journal
Ulysses 6
Hemispheric distribution of coronal mass ejections from 1996 to 2020
DOI: 10.1093/mnras/stad323 Bibcode: 2023MNRAS.520.3923Z

Li, C.; Deng, L. H.; Zhang, X. J. +3 more

Solar magnetic structures are known to be asymmetrically distributed between the two hemispheres. To date, the hemispheric variations of the coronal mass ejections (CMEs) at different latitudes, in different cycles, and for different types (regular and specific events) are still unclear. From the list of white-light CMEs in the Coordinated Data An…

2023 Monthly Notices of the Royal Astronomical Society
SOHO 6
Kinematics of stellar substructures in the small magellanic cloud
DOI: 10.1093/mnras/stad1339 Bibcode: 2023MNRAS.523..347E

de Grijs, Richard; Kacharov, Nikolay; Cioni, Maria-Rosa L. +6 more

We present a kinematic analysis of the Small Magellanic Cloud using 3700 spectra extracted from the European Southern Observatory archive. We used data from Gaia and near-infrared photometry to select stellar populations and discard Galactic foreground stars. The sample includes main-sequence red giant branch and red clump stars, observed with Fib…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6
Retrieval of Martian Atmospheric CO Vertical Profiles From NOMAD Observations During the First Year of TGO Operations
DOI: 10.1029/2022JE007282 Bibcode: 2023JGRE..12807282M

Modak, Ashimananda; López-Valverde, Miguel Angel; Brines, Adrian +19 more

We present CO density profiles up to about 100 km in the Martian atmosphere obtained for the first time from retrievals of solar occultation measurements by the Nadir and Occultation for Mars Discovery (NOMAD) onboard ExoMars Trace Gas Orbiter (TGO). CO is an important trace gas on Mars, as it is controlled by CO2 photolysis, chemical r…

2023 Journal of Geophysical Research (Planets)
ExoMars-16 6
PIC Simulations of Overstretched Ion-Scale Current Sheets in the Magnetotail
DOI: 10.1029/2023GL104534 Bibcode: 2023GeoRL..5004534A

Arnold, H.; Sitnov, M. I.

Onset of reconnection in the tail requires the current sheet thickness to be of the order of the ion thermal gyroradius or smaller. However, existing isotropic plasma models cannot explain the formation of such thin sheets at distances where the X-lines are typically observed. Here we reproduce such thin and long sheets in particle-in-cell simulat…

2023 Geophysical Research Letters
Cluster 6
Multi-epoch hard X-ray view of Compton-thick AGN Circinus Galaxy
DOI: 10.1093/mnras/stad1216 Bibcode: 2023MNRAS.522.4098K

Gandhi, Poshak; Ricci, Claudio; Kayal, Abhijit +4 more

The circumnuclear material around active galactic nuclei (AGNs) is one of the essential components of the obscuration-based unification model. However, our understanding of the circumnuclear material in terms of its geometrical shape, structure, and its dependence on accretion rate is still debated. In this paper, we present the multi-epoch broad-…

2023 Monthly Notices of the Royal Astronomical Society
Suzaku XMM-Newton 6
An XMM-Newton View of the Symbiotic Stars HM Sge, NQ Gem, and PU Vul
DOI: 10.3847/1538-4357/acc659 Bibcode: 2023ApJ...948...14T

Toalá, Jesús A.; Sabin, Laurence; Botello, Marissa K.

We present the analysis of archival XMM-Newton observations of the symbiotic stars HM Sge, NQ Gem, and PU Vul. The EPIC-pn spectra hint at the presence of emission lines, which are further confirmed in the first-order RGS spectra of the three sources. Spectral modeling of the EPIC-pn data discloses unprecedented characteristics; for instance, the …

2023 The Astrophysical Journal
XMM-Newton 6
Discovery and characterization of two Neptune-mass planets orbiting HD 212729 with TESS
DOI: 10.1093/mnras/stad2183 Bibcode: 2023MNRAS.524.5804A

Torres, Guillermo; Latham, David W.; Wheatley, Peter J. +33 more

We report the discovery of two exoplanets orbiting around HD 212729 (TOI 1052, TIC 317060587), a Teff = 6146 K star with V = 9.51 observed by TESS in Sectors 1 and 13. One exoplanet, TOI-1052b, is Neptune-mass and transits the star, and an additional planet TOI-1052c is observed in radial velocities but not seen to transit. We confirm t…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6
Further Evidence for the 9 s Pulsation in LS 5039 from NuSTAR and ASCA
DOI: 10.3847/1538-4357/ad0bdf Bibcode: 2023ApJ...959...79M

Enoto, Teruaki; Makishima, Kazuo; Takahashi, Tadayuki +2 more

The present study aims to reinforce the evidence for the ~9 s pulsation in the gamma-ray binary LS 5039, derived from a Suzaku observation in 2007 and a NuSTAR observation in 2016. Through a reanalysis of the NuSTAR data incorporating the orbital Doppler correction, the 9.0538 s pulsation was confirmed successfully even in the 3-10 keV range, wher…

2023 The Astrophysical Journal
Suzaku 6