Search Publications

Changes in the Na D1 Absorption Components of η Carinae Provide Clues on the Location of the Dissipating Central Occulter
DOI: 10.3847/1538-4357/ac898f Bibcode: 2022ApJ...937...85P

Moffat, Anthony F. J.; Hillier, D. John; Gull, Theodore R. +9 more

The Na D absorption doublet in the spectrum of η Carinae is complex, with multiple absorption features associated with the Great Eruption (1840s), the Lesser Eruption (1890s), and the interstellar clouds. The velocity profile is further complicated by the P Cygni profile originating in the system's stellar winds and blending with the He I λ5876 pr…

2022 The Astrophysical Journal
eHST 6
Identifying the 3FHL Catalog. VI. Swift Observations of 3FHL Unassociated Objects with Source Classification via Machine Learning
DOI: 10.3847/1538-4357/ac9797 Bibcode: 2022ApJ...940..139J

Ajello, M.; Marchesi, S.; Torres-Albà, N. +5 more

The Third Catalog of Hard Fermi Large Area Telescope Sources (3FHL) reports the detection of 1556 objects at E > 10 GeV. However, 177 sources remain unassociated and 23 are associated with a ROSAT X-ray detection of unknown origin. Pointed X-ray observations were conducted on 30 of these unassociated and unknown sources with Swift-XRT. A bright…

2022 The Astrophysical Journal
Gaia XMM-Newton 6
The Global Structure of the Milky Way's Stellar Halo Based on the Orbits of Local Metal-poor Stars
DOI: 10.3847/1538-4357/ac47fb Bibcode: 2022ApJ...927..145S

Chiba, Masashi; Sato, Genta

We analyze the global structure of the Milky Way (MW)'s stellar halo, including its dominant subcomponent, Gaia-Sausage-Enceladus (GSE). The method for reconstructing the global distribution of this old stellar component is to employ the superposition of the orbits covering the large MW's space, where each of the orbit-weighting factors is assigne…

2022 The Astrophysical Journal
Gaia 6
The Physical Properties of Massive Green Valley Galaxies as a Function of Environments at 0.5 < z < 2.5 in 3D-HST/Candels Fields
DOI: 10.3847/1538-4357/ac8748 Bibcode: 2022ApJ...936...47C

Fang, Guanwen; Lin, Zesen; Kong, Xu +3 more

To investigate the effects of environment in the quenching phase, we study the empirical relations for green valley (GV) galaxies between overdensity and other physical properties (i.e., effective radius r e , Sérsic indices n, and specific star formation rate (sSFR)). Based on five 3D-HST/CANDELS fields, we construct a large sample of …

2022 The Astrophysical Journal
eHST 6
A Massive AGB Donor in Scutum X-1: Identification of the First Mira Variable in an X-Ray Binary
DOI: 10.3847/2041-8213/ac5b11 Bibcode: 2022ApJ...928L...8D

Soria, Roberto; Conroy, Charlie; Chakrabarty, Deepto +9 more

The symbiotic X-ray binary Sct X-1 was suggested to be the first known neutron star accreting from a red supergiant companion. Although known for nearly 50 yr, detailed characterization of the donor remains lacking, particularly due to the extremely high reddening toward the source (A V ≳ 25 mag). Here, we present (i) improved localiz…

2022 The Astrophysical Journal
Gaia 6
ALMA Observations of CO Emission from Luminous Lyman-break Galaxies at z = 6.0293-6.2037
DOI: 10.3847/1538-4357/ac9ea6 Bibcode: 2022ApJ...941...74O

Ono, Yoshiaki; Ouchi, Masami; Fujimoto, Seiji +14 more

We present our new Atacama Large Millimeter/submillimeter Array (ALMA) observations targeting CO(6-5) emission from three luminous Lyman-break galaxies (LBGs) at z spec = 6.0293-6.2037 found in the Subaru/Hyper Suprime-Cam survey, whose [O III] 88 µm and [C II] 158 µm emissions have been detected with ALMA. We find a margina…

2022 The Astrophysical Journal
Gaia 6
Explanation of Heliospheric Energetic Neutral Atom Fluxes Observed by the Interstellar Boundary Explorer
DOI: 10.3847/2041-8213/ac92e2 Bibcode: 2022ApJ...937L..38Z

McComas, D. J.; Rankin, J. S.; Dayeh, M. A. +3 more

Interstellar neutral atoms propagating into the heliosphere experience charge exchange with the supersonic solar wind (SW) plasma, generating ions that are picked up by the SW. These pickup ions (PUIs) constitute ~25% of the proton number density by the time they reach the heliospheric termination shock (HTS). Preferential acceleration of PUIs at …

2022 The Astrophysical Journal
Ulysses 6
Variations of the Internal Asymmetries of Sunspot Groups during Their Decay
DOI: 10.3847/1538-4357/ac3de6 Bibcode: 2022ApJ...925...87M

Muraközy, Judit

The aim of the present study is to show the varying asymmetries during the decay of sunspot groups. The source of input data is the SOHO/MDI-Debrecen Database sunspot catalog that contains the magnetic polarity data for time interval 1996-2010. Several types of asymmetries were examined on the selected sample of 142 sunspot groups. The leading-fol…

2022 The Astrophysical Journal
SOHO 6
No Evolution in the Half-mass Radius of Milky Way-type Galaxies over the Last 10 Gyr
DOI: 10.3847/2041-8213/ac76c8 Bibcode: 2022ApJ...932L..23H

Tacchella, Sandro; Park, Minjung; Naidu, Rohan P. +3 more

The Milky Way (MW) galaxy is in focus, thanks to new observational data. Here we shed new light on the MW's past by studying the structural evolution of MW progenitors, which we identify from extragalactic surveys. Specifically, we constrain the stellar-mass growth history (SMGH) of the MW with two methods: (i) direct measurement of the MW's star …

2022 The Astrophysical Journal
eHST 6
Ages of Main-sequence Turnoff Stars from the GALAH Survey
DOI: 10.3847/1538-4357/ac55a1 Bibcode: 2022ApJ...929..124C

Wu, Yaqian; Chen, Yuqin; Bi, Shaolan +6 more

Main-sequence turnoff (MSTO) stars are good tracers of Galactic populations since their ages can be reliably estimated from atmospheric parameters. Based on the GALAH survey, we use the Yale rotation evolution code to determine the ages of 2926 MSTO stars with a mean age uncertainty of ~10% considering the variation of C and O abundances. The ages…

2022 The Astrophysical Journal
Gaia 6