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On the Variation in the Volumetric Evolution of CMEs from the Inner to Outer Corona
DOI: 10.3847/1538-4357/ac5909 Bibcode: 2022ApJ...929...11M

Pant, Vaibhav; Patel, Ritesh; Majumdar, Satabdwa

Some of the major challenges faced in understanding the early evolution of coronal mass ejections (CMEs) are due to the limited observations in the inner corona (<3 R ) and the plane-of-sky measurements. In this work, we have thus extended the application of the Graduated Cylindrical Shell (GCS) model to inner coronal observations f…

2022 The Astrophysical Journal
SOHO 11
The peculiar chemical abundance of the transitional millisecond pulsar PSR J1023+0038 - Li enhancement
DOI: 10.1093/mnras/stac492 Bibcode: 2022MNRAS.513...71S

Breton, R. P.; Kennedy, M. R.; Mata Sánchez, D. +3 more

Using high-resolution optical spectroscopy we determine the chemical abundance of the secondary star in the binary millisecond pulsar PSR J1023+0038. We measure a metallicity of [Fe/H] = 0.48 ± 0.04 which is higher than the Solar value and in general find that the element abundances are different compared to the secondary stars in X-ray binaries a…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 11
The Fractality and Size Distributions of Astrophysical Self-Organized Criticality Systems
DOI: 10.3847/1538-4357/ac6bf2 Bibcode: 2022ApJ...934...33A

Aschwanden, Markus J.

The statistics of nonlinear processes in avalanching systems, based on the self-organized criticality (SOC) concept of Bak et al. (1988), predicts power-law-like size (or occurrence frequency) distribution functions. Following up on previous work, we define a standard SOC model in terms of six assumptions: (i) area fractality, (ii) volume fractali…

2022 The Astrophysical Journal
Ulysses 11
Prediction of Astrometric-microlensing Events from Gaia eDR3 Proper Motions
DOI: 10.3847/1538-3881/ac4fc0 Bibcode: 2022AJ....163..176K

Bastian, Ulrich; Wambsganss, Joachim; Klüter, Jonas +1 more

Astrometric microlensing is a unique tool to measure stellar masses. It allows us to determine the mass of the lensing star with an accuracy of a few percent. In this paper, we update, extend, and refine our predictions of astrometric-microlensing events based on Gaia's early Data release 3 (eDR3). We selected about 500.000 high-proper-motion star…

2022 The Astronomical Journal
Gaia 11
Unveiling the Nature of SN 2011fh: A Young and Massive Star Gives Rise to a Luminous SN 2009ip-like Event
DOI: 10.3847/1538-4357/ac562d Bibcode: 2022ApJ...928..138P

Kochanek, Christopher S.; Prieto, Jose L.; Fox, Ori D. +6 more

In recent years, many Type IIn supernovae have been found to share striking similarities with the peculiar SN 2009ip, whose true nature is still under debate. Here, we present 10 yr of observations of SN 2011fh, an interacting transient with spectroscopic and photometric similarities to SN 2009ip. SN 2011fh had an M r ~ -16 mag bright…

2022 The Astrophysical Journal
eHST 11
The Role of Magnetic Fields in Triggered Star Formation of RCW 120
DOI: 10.1088/1674-4527/ac6f4c Bibcode: 2022RAA....22g5017C

Chen, Zhiwei; Sefako, Ramotholo; Jiang, Zhibo +3 more

We report on the near-infrared polarimetric observations of RCW 120 with the 1.4 m IRSF telescope. The starlight polarization of the background stars reveals for the first time the magnetic field of RCW 120. The global magnetic field of RCW 120 is along the direction of 20°, parallel to the Galactic plane. The field strength on the plane of the sk…

2022 Research in Astronomy and Astrophysics
Gaia 11
The search for gas in debris discs: ALMA detection of CO gas in HD 36546
DOI: 10.1093/mnras/stab2906 Bibcode: 2022MNRAS.509..693R

Henning, Thomas; Villaver, Eva; Rivière-Marichalar, Pablo +9 more

Debris discs represent the last stages of planet formation and as such are expected to be depleted of primordial gas. None the less, in the last few years the presence of cold gas has been reported in ~20 debris discs from far-infrared to (sub-)mm observations and hot gas has been observed in the optical spectra of debris discs for decades. While …

2022 Monthly Notices of the Royal Astronomical Society
AKARI Gaia Herschel 11
The Disk-Outflow System around the Rare Young O-type Protostar W42-MME
DOI: 10.3847/1538-4357/ac36dd Bibcode: 2022ApJ...925...41D

Dewangan, L. K.; Ojha, D. K.; Mayya, Y. D. +6 more

We present line and continuum observations (resolution ~0.″3-3.″5) made with the Atacama Large Millimeter/submillimeter Array (ALMA), Submillimeter Array, and Very Large Array of a young O-type protostar W42-MME (mass: 19 ± 4 M ). The ALMA 1.35 mm continuum map (resolution ~1″) shows that W42-MME is embedded in one of the cores (i.e., …

2022 The Astrophysical Journal
Herschel 11
A census of post-AGB stars in Gaia DR3: evidence for a substantial population of Galactic post-RGB stars
DOI: 10.1093/mnrasl/slac088 Bibcode: 2022MNRAS.516L..61O

Oudmaijer, René D.; Jones, Emma R. M.; Vioque, Miguel

This paper presents the first census of Galactic post-asymptotic giant branch (post-AGB) stars in the Hertzsprung-Russell (HR) diagram. We combined Gaia DR3 parallax-based distances with extinction corrected integrated fluxes and derived luminosities for a sample of 185 stars that had been proposed to be post-AGB stars in the literature. The lumin…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 11
Disambiguation of Vector Magnetograms by Stereoscopic Observations from the Solar Orbiter (SO)/Polarimetric and Helioseismic Imager (PHI) and the Solar Dynamic Observatory (SDO)/Helioseismic and Magnetic Imager (HMI)
DOI: 10.1007/s11207-021-01942-x Bibcode: 2022SoPh..297...12V

Hirzberger, Johann; Valori, Gherardo; Chen, Feng +3 more

Spectropolarimetric reconstructions of the photospheric vector magnetic field are intrinsically limited by the 180 ambiguity in the orientation of the transverse component. The successful launch and operation of Solar Orbiter have made the removal of the 180 ambiguity possible using solely observations obtained from two dif…

2022 Solar Physics
SolarOrbiter 11