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Phenomenology of CP-even ALP
DOI: 10.1007/JHEP04(2022)113 Bibcode: 2022JHEP...04..113S

Sakurai, Kodai; Yin, Wen

Axion or axion-like particle (ALP) has been usually considered as a CP-odd Nambu-Goldstone boson (NGB) from the spontaneous breakdown of a global U(1) symmetry. In this paper, we point out that the NGB behaves as a CP-even particle coupled to the SM particles in a large class of simple (or perhaps the simplest) renormalizable models. We provide a …

2022 Journal of High Energy Physics
INTEGRAL 15
TOI-1268b: The youngest hot Saturn-mass transiting exoplanet
DOI: 10.1051/0004-6361/202142883 Bibcode: 2022A&A...662A.107S

Fridlund, M.; Pallé, E.; Guenther, E. W. +41 more

We report the discovery of TOI-1268b, a transiting Saturn-mass planet from the TESS space mission. With an age of less than 1 Gyr, derived from various age indicators, TOI-1268b is the youngest Saturn-mass planet known to date; it contributes to the small sample of well-characterised young planets. It has an orbital period of P = 8.1577080 ± 0.000…

2022 Astronomy and Astrophysics
AKARI Gaia 15
A Dearth of Close-in Stellar Companions to M-dwarf TESS Objects of Interest
DOI: 10.3847/1538-3881/ac6101 Bibcode: 2022AJ....163..232C

Howell, Steve B.; Beichman, Charles A.; Ciardi, David R. +5 more

TESS has proven to be a powerful resource for finding planets, including those that orbit the most prevalent stars in our galaxy: M dwarfs. Identification of stellar companions (both bound and unbound) has become a standard component of the transiting planet confirmation process in order to assess the level of light-curve dilution and the possibil…

2022 The Astronomical Journal
Gaia 15
Microlensing and the type Ia supernova iPTF16geu
DOI: 10.1051/0004-6361/202143009 Bibcode: 2022A&A...662A..34D

Diego, J. M.; Goobar, A.; Mörtsell, E. +5 more

The observed magnifications and light curves of the quadruply imaged iPTF16geu supernova (SN) offers a unique opportunity to study a lens system with a variety of independent constraints. The four observed positions can be used to constrain the macrolens model. The magnifications and light curves at the four SN positions are more useful to constra…

2022 Astronomy and Astrophysics
eHST 15
In-depth direct imaging and spectroscopic characterization of the young Solar System analog HD 95086
DOI: 10.1051/0004-6361/202243097 Bibcode: 2022A&A...664A.139D

Rouan, D.; Ménard, F.; Henning, T. +48 more

Context. HD 95086 is a young nearby Solar System analog hosting a giant exoplanet orbiting at 57 au from the star between an inner and outer debris belt. The existence of additional planets has been suggested as the mechanism that maintains the broad cavity between the two belts.
Aims: We present a dedicated monitoring of HD 95086 with the VL…

2022 Astronomy and Astrophysics
Gaia 15
Revealing the Field Sub-subgiant Population Using a Catalog of Active Giant Stars and Gaia EDR3
DOI: 10.3847/1538-4357/ac53b1 Bibcode: 2022ApJ...927..222L

Tofflemire, Benjamin M.; Gully-Santiago, Michael A.; Geller, Aaron M. +2 more

Sub-subgiant stars (SSGs) fall below the subgiant branch and/or red of the giant branch in open and globular clusters, an area of the color-magnitude diagram (CMD) not populated by standard stellar evolution tracks. One hypothesis is that SSGs result from rapid rotation in subgiants or giants due to tidal synchronization in a close binary. The str…

2022 The Astrophysical Journal
Gaia 15
Spectral analysis of cool white dwarfs accreting from planetary systems: from the ultraviolet to the optical
DOI: 10.1093/mnras/stab3696 Bibcode: 2022MNRAS.511...71H

Gänsicke, B. T.; Tremblay, P. -E.; Hollands, M. A. +1 more

The accretion of planetary debris into the atmospheres of white dwarfs leads to the presence of metal lines in their spectra. Cool metal-rich white dwarfs, which left the main sequence many Gyr ago, allow the study of the remnants of the oldest planetary systems. Despite their low effective temperatures (Teff), a non-negligible amount o…

2022 Monthly Notices of the Royal Astronomical Society
eHST 15
MICROSCOPE mission: data analysis principle
DOI: 10.1088/1361-6382/ac0235 Bibcode: 2022CQGra..39t4007B

Bergé, Joel; Chhun, Ratana; Métris, Gilles +10 more

After performing highly sensitive acceleration measurements during two years of drag-free flight around the Earth, MICROSCOPE provided the best constraint on the weak equivalence principle (WEP) to date. Beside being a technological challenge, this experiment required a specialised data analysis pipeline to look for a potential small signal buried…

2022 Classical and Quantum Gravity
MICROSCOPE 15
The Planetary Nebula in the 500 Myr Old Open Cluster M37
DOI: 10.3847/2041-8213/ac88c1 Bibcode: 2022ApJ...935L..35F

Parker, Quentin A.; Sabin, Laurence; Zijlstra, Albert A. +3 more

We report confirmation of a large, evolved, bipolar planetary nebula and its blue, white dwarf central star as a member of the ~500 Myr old Galactic open star cluster M37 (NGC 2099). This is only the third known example of a planetary nebula in a Galactic open cluster and was found via our ongoing program of identifying and studying planetary nebu…

2022 The Astrophysical Journal
Gaia 15
Structure and evolution of ultra-massive white dwarfs in general relativity
DOI: 10.1051/0004-6361/202244604 Bibcode: 2022A&A...668A..58A

Córsico, Alejandro H.; Rebassa-Mansergas, Alberto; Althaus, Leandro G. +4 more

Context. Ultra-massive white dwarfs (M ≳ 1.05 M) are of utmost importance in view of the role they play in type Ia supernovae explosions, merger events, the existence of high-magnetic -field white dwarfs, and the physical processes in the super asymptotic giant branch phase.
Aims: We aim to present the first set of con…

2022 Astronomy and Astrophysics
Gaia 15