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Searching for C II Emission from the First Sample of z ∼ 6 O I Absorption-associated Galaxies with the Atacama Large Millimeter/submillimeter Array
DOI: 10.3847/1538-4357/ad00b8 Bibcode: 2023ApJ...958...16W

Hennawi, Joseph F.; Fan, Xiaohui; Prochaska, J. Xavier +13 more

We report the first statistical analyses of [C II] and dust continuum observations in six strong O I absorber fields at the end of the reionization epoch obtained by the Atacama Large Millimeter/submillimeter Array (ALMA). Combined with one [C II] emitter reported in Wu et al., we detect one O I-associated [C II] emitter in six fields. At redshift…

2023 The Astrophysical Journal
eHST 3
Atomic oxygen abundance toward Sagittarius B2
DOI: 10.1051/0004-6361/202245481 Bibcode: 2023A&A...669L..15L

Wiesemeyer, Helmut; Güsten, Rolf; Seo, Youngmin +4 more

A substantial fraction of oxygen in diffuse clouds is unaccounted for by observations and is postulated to be in an unknown refractory form, referred to as unidentified depleted oxygen (UDO), which, depending on the local gas density, may contribute up to 50% of the total oxygen content. Previous Infrared Space Observatory (ISO) observations sugge…

2023 Astronomy and Astrophysics
Herschel ISO 3
Eight Exoplanet Candidates in SAO Survey
DOI: 10.1134/S1990341323010108 Bibcode: 2023AstBu..78...79Y

Galazutdinov, G. A.; Beskin, G. M.; Romanyuk, I. I. +15 more

We report eight new exoplanet candidates discovered at the Special Astrophysical Observatory of the Russian Academy of Sciences using the transit technique. Photometric observations were performed with a 50-cm robotic telescope during the second half of 2020. Transits with depths of $$\Delta m=0\ov…

2023 Astrophysical Bulletin
Gaia 3
X-Ray Studies of Blazar 1ES 1959+650 Using Swift and XMM-Newton Satellite
DOI: 10.3847/1538-4357/acd186 Bibcode: 2023ApJ...951...94W

Gaur, Haritma; Wani, Kiran; Patil, M. K.

High synchrotron energy peaked blazar 1ES 1959+650 was studied with the Swift and XMM-Newton satellites in a total of 127 observations during the period 2018 June-2020 December. We extensively studied its flux and spectral variability on intraday and long-term timescales. Discrete correlation function analysis between soft and hard X-ray bands ind…

2023 The Astrophysical Journal
XMM-Newton 3
The Cycles of Alpha Centauri: Double Dipping of AB
DOI: 10.3847/1538-3881/acfef5 Bibcode: 2023AJ....166..212A

Ayres, Thomas

In mid-2023, the Sunlike dwarfs of nearby α Centauri (HD 128620 ("A"): G2 V; HD 128621 ("B"): K1 V; hereafter "AB") coincidentally both entered coronal (T ≈ 1-3 MK) low states in their long-term X-ray cycles, as captured by the Chandra Observatory and its High Resolution Camera (HRC-I). The assessment benefited from a sensitivity degradation model…

2023 The Astronomical Journal
XMM-Newton eHST 3
Forming stars in a dual AGN host: molecular and ionized gas in the nearby, luminous infrared merger, Mrk 266
DOI: 10.1093/mnras/stac3048 Bibcode: 2023MNRAS.518.1407B

Robert, Carmelle; Rousseau-Nepton, Laurie; Heckman, Timothy +5 more

We present star formation rates based on cold and ionized gas measurements of Mrk 266 (NGC 5256), a system composed of two colliding gas-rich galaxies, each hosting an active galactic nucleus. Using 12CO (1-0) observations with the Combined Array for Research in Millimeter-Wave Astronomy (CARMA), we find a total H2 mass in th…

2023 Monthly Notices of the Royal Astronomical Society
Herschel 3
Modified Masses and Parallaxes of Close Binary Systems: HD 39438
DOI: 10.1088/1674-4527/ace51b Bibcode: 2023RAA....23k5005M

Masda, Suhail; Yousef, Z. T.; Al-Wardat, Mashhoor +1 more

We present the detailed fundamental stellar parameters of the close visual binary system HD 39438 for the first time. We used Al-Wardat's method for analyzing binary and multiple stellar systems. The method implements Kurucz's plane parallel model atmospheres to construct synthetic spectral energy distributions (SEDs) for both components of the sy…

2023 Research in Astronomy and Astrophysics
Gaia 3
Photometric variations from stellar activity as an age indicator for solar-twins
DOI: 10.1093/mnras/stad1085 Bibcode: 2023MNRAS.522.2675P

Yana Galarza, Jhon; Lorenzo-Oliveira, Diego; Valio, Adriana +2 more

Stellar ages are elusive to measure, albeit being very important for understanding stellar evolution. We investigate the impact of photospheric activity on 2-min cadence light curves from the TESS/NASA mission of a selected sample of 30 solar-twins with well-determined ages. The photometric variability, $\mathcal {A}_{ {{TESS}}}$, of the light cur…

2023 Monthly Notices of the Royal Astronomical Society
SOHO 3
Numerical Prediction of Changes in Atmospheric Chemical Compositions During a Solar Energetic Particle Event on Mars
DOI: 10.1029/2022JA031250 Bibcode: 2023JGRA..12831250N

Leblanc, François; Vandaele, Ann Carine; Aoki, Shohei +11 more

Precipitation of solar energetic particles (SEPs) into planetary atmospheres causes changes in atmospheric chemical composition through ionization, dissociation, and excitation of atmospheric molecules. In contrast to the terrestrial atmosphere, where depletion of ozone in the polar mesosphere has been studied by observations and models for decade…

2023 Journal of Geophysical Research (Space Physics)
ExoMars-16 3
The magnetic fields around the cometary globules L328, L323, and L331
DOI: 10.1093/mnras/stad1845 Bibcode: 2023MNRAS.524.1219K

Soam, Archana; Roy, Nirupam; Kumar, Siddharth

This work presents the magnetic field geometry in a complex of three cometary (with head-tail morphology) globules, namely LDN 323, LDN 328, and LDN 331, using R-band polarization measurements of background stars. These observations were combined with a Planck sky survey to study the large-scale morphology of the magnetic fields in the region. The…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 3