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Limits on X-Ray Polarization at the Core of Centaurus A as Observed with the Imaging X-Ray Polarimetry Explorer
DOI: 10.3847/1538-4357/ac8056 Bibcode: 2022ApJ...935..116E

Wu, Kinwah; Enoto, Teruaki; Turolla, Roberto +96 more

We present measurements of the polarization of X-rays in the 2-8 keV band from the nucleus of the radio galaxy Centaurus A (Cen A), using a 100 ks observation from the Imaging X-ray Polarimetry Explorer (IXPE). Nearly simultaneous observations of Cen A were also taken with the Swift, NuSTAR, and INTEGRAL observatories. No statistically significant…

2022 The Astrophysical Journal
INTEGRAL 19
The Astrophysical Distance Scale. V. A 2% Distance to the Local Group Spiral M33 via the JAGB Method, Tip of the Red Giant Branch, and Leavitt Law
DOI: 10.3847/1538-4357/ac7321 Bibcode: 2022ApJ...933..201L

Rousseau-Nepton, Laurie; Madore, Barry F.; Freedman, Wendy L. +6 more

The J-region asymptotic giant branch (JAGB) method is a new standard candle that is based on the stable intrinsic J-band magnitude of color-selected carbon stars, and has a precision comparable to other primary distance indicators such as Cepheids and the TRGB. We further test the accuracy of the JAGB method in the Local Group galaxy M33. M33's mo…

2022 The Astrophysical Journal
eHST 19
A Fresh Look at AGB Stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
DOI: 10.3847/1538-4365/ac374a Bibcode: 2022ApJS..258...43M

Girardi, Léo; Cummings, Jeffrey D.; Marigo, Paola +7 more

Benefiting from the Gaia second and early third releases of photometric and astrometric data, we examine the population of asymptotic giant branch (AGB) stars that appear in the fields of intermediate-age and young open star clusters. We identify 49 AGB star candidates, brighter than the tip of the red giant branch, with a good to high cluster mem…

2022 The Astrophysical Journal Supplement Series
Gaia 19
Probable dormant neutron star in a short-period binary system
DOI: 10.1093/mnras/stac2853 Bibcode: 2022MNRAS.517.4005M

Maoz, Dan; Latham, David W.; Liu, Jifeng +24 more

We have identified 2XMM J125556.57+565846.4, at a distance of 600 pc, as a binary system consisting of a normal star and a probable dormant neutron star. Optical spectra exhibit a slightly evolved F-type single star, displaying periodic Doppler shifts with a 2.76-d Keplerian circular orbit, with no indication of light from a secondary component. O…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 19
First Detection of Transverse Vertical Oscillation during the Expansion of Coronal Loops
DOI: 10.3847/2041-8213/ac8e01 Bibcode: 2022ApJ...937L..21Z

Li, Dong; Zhang, Qingmin; Li, Chuan +3 more

In this Letter, we perform a detailed analysis of the M5.5 class eruptive flare occurring in active region 12,929 on 2022 January 20. The eruption of a hot channel generates a fast coronal mass ejection (CME) and a dome-shaped extreme-ultraviolet (EUV) wave at speeds of 740-860 km s-1. The CME is associated with a type II radio burst, i…

2022 The Astrophysical Journal
SOHO 19
Sensitivity to dark sector scales from gravitational wave signatures
DOI: 10.1007/JHEP08(2022)300 Bibcode: 2022JHEP...08..300D

Dent, James B.; Dutta, Bhaskar; Ghosh, Sumit +2 more

We consider gravitational sound wave signals produced by a first-order phase transition in a theory with a generic renormalizable thermal effective potential of power law form. We find the frequency and amplitude of the gravitational wave signal can be related in a straightforward manner to the parameters of the thermal effective potential. This l…

2022 Journal of High Energy Physics
Gaia 18
The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2
DOI: 10.3847/1538-4357/ac99e0 Bibcode: 2022ApJ...941...51H

Zhang, Yapeng; Pattle, Kate; Karoly, Janik +157 more

We present and analyze observations of polarized dust emission at 850 µm toward the central 1 × 1 pc hub-filament structure of Monoceros R2 (Mon R2). The data are obtained with SCUBA-2/POL-2 on the James Clerk Maxwell Telescope (JCMT) as part of the B-fields in Star-forming Region Observations survey. The orientations of the magnetic field f…

2022 The Astrophysical Journal
Herschel 18
The Heliosphere and Local Interstellar Medium from Neutral Atom Observations at Energies Below 10 keV
DOI: 10.1007/s11214-022-00901-7 Bibcode: 2022SSRv..218...31G

Schwadron, Nathan A.; Izmodenov, Vladislav V.; Kucharek, Harald +8 more

As the heliosphere moves through the surrounding interstellar medium, a fraction of the interstellar neutral helium, hydrogen, and heavier species crossing the heliopause make it to the inner heliosphere as neutral atoms with energies ranging from few eV to several hundred eV. In addition, energetic neutral hydrogen atoms originating from solar wi…

2022 Space Science Reviews
SOHO Ulysses 18
Pulsating B stars in the Scorpius-Centaurus Association with TESS
DOI: 10.1093/mnras/stac1816 Bibcode: 2022MNRAS.515..828S

Bedding, Timothy R.; White, Timothy R.; Saio, Hideyuki +1 more

We study 119 B stars located in the Scorpius-Centaurus Association using data from NASA's TESS Mission. We see pulsations in 81 stars (68 per cent) across the full range of effective temperatures. In particular, we confirm previous reports of low-frequency pulsations in stars whose temperatures fall between the instability strips of SPB stars (slo…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 18
An extended stellar halo discovered in the Fornax dwarf spheroidal using Gaia EDR3
DOI: 10.1093/mnras/stac644 Bibcode: 2022MNRAS.512.4171Y

Hammer, François; Pawlowski, Marcel S.; Yang, Yanbin +1 more

We have studied the extent of the Red Giant Branch stellar population in the Fornax dwarf spheroidal galaxy using the spatially extended and homogeneous data set from Gaia EDR3. Our pre-selection of stars belonging to Fornax is based on their proper motions, parallaxes, and colour-magnitude diagram. The latter criteria provide a Fornax star sample…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 18