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The "Singular" Behavior of the Solar Wind Scaling Features during Parker Solar Probe-BepiColombo Radial Alignment
DOI: 10.3847/1538-4357/ac478d Bibcode: 2022ApJ...926..174A

Richter, Ingo; Auster, Hans-Ulrich; Hadid, Lina Z. +4 more

At the end of 2020 September, the Parker Solar Probe (PSP) and BepiColombo were radially aligned: PSP was orbiting near 0.17 au and BepiColombo near 0.6 au. This geometry is of particular interest for investigating the evolution of solar wind properties at different heliocentric distances by observing the same solar wind plasma parcels. In this wo…

2022 The Astrophysical Journal
BepiColombo 13
The Initial-Final Mass Relation of White Dwarfs: A Tool to Calibrate the Third Dredge-Up
DOI: 10.3390/universe8040243 Bibcode: 2022Univ....8..243M

Marigo, Paola

The initial mass-final mass relationship (IFMR) of white dwarfs (WD) represents a crucial benchmark for stellar evolution models, especially for the efficiency of mixing episodes and mass loss during the asymptotic giant branch (AGB) phase. In this study, we argue that this relation offers the opportunity to constrain the third dredge-up (3DU), wi…

2022 Universe
Gaia 13
The magnetic field and magnetosphere of Plaskett's star: a fundamental shift in our understanding of the system
DOI: 10.1093/mnras/stab3320 Bibcode: 2022MNRAS.512.1944G

Wade, G. A.; Neiner, C.; Alecian, E. +7 more

Plaskett's 'star' appears to be one of a small number of short-period binary systems known to contain a hot, massive, magnetic star. We combine an extensive spectropolarimetric (Stokes V) data set with archival photometry and spectropolarimetry to establish the essential characteristics of the magnetic field and magnetosphere of the rapidly rotati…

2022 Monthly Notices of the Royal Astronomical Society
CoRoT Gaia 13
X-ray timing and spectral variability properties of blazars S5 0716 + 714, OJ 287, Mrk 501, and RBS 2070
DOI: 10.1093/mnras/stab3738 Bibcode: 2022MNRAS.510.5280M

Mohorian, Maksym; Bhatta, Gopal; Adhikari, Tek P. +6 more

The X-ray emission from blazars has been widely investigated using several space telescopes. In this work, we explored statistical properties of the X-ray variability in the blazars S5 0716+714, OJ 287, Mkn 501, and RBS 2070 using the archival observations from the XMM-Newton telescope between the period 2002-2020. Several methods of timing and sp…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 13
A Gaia View on the Star Formation in the Monoceros OB1 and R1 Associations
DOI: 10.3847/1538-3881/ac63b6 Bibcode: 2022AJ....163..266L

Lim, Beomdu; Lee, Jeong-Eun; Park, Byeong-Gon +5 more

Stellar kinematics provides the key to understanding the star formation process. In this respect, we present a kinematic study of the Monoceros OB1 (Mon OB1) and R1 (Mon R1) associations using the recent Gaia data and radial velocities of stars derived from high-resolution spectroscopy and the literature. A total of 728 members are selected using …

2022 The Astronomical Journal
AKARI Gaia 13
A Partial Filament Eruption in Three Steps Induced by External Magnetic Reconnection
DOI: 10.3847/1538-4357/ac4fbe Bibcode: 2022ApJ...929...85D

Xu, Zhe; Li, Leping; Zhang, Qingmin +6 more

We present an investigation of partial filament eruption on 2012 June 17 in the active region NOAA 11504. For the first time, we observed the vertical splitting process during the partial eruption with high-resolution narrowband images at 10830 Å. The active filament was rooted in a small δ-sunspot of the active region. Particularly, it underwent …

2022 The Astrophysical Journal
SOHO 13
The Lyman Alpha Reference Sample. XII. Morphology of extended Lyman alpha emission in star-forming galaxies
DOI: 10.1051/0004-6361/202140734 Bibcode: 2022A&A...662A..64R

Östlin, G.; Hayes, M.; Kunth, D. +7 more


Aims: We use Hubble Space Telescope data of 45 nearby star-forming galaxies to investigate properties of Lyman-alpha (Lyα) halos, Lyα morphology, and the star-forming characteristics of galaxies. We study how the morphology of Lyα emission is related to other Lyα observables. Furthermore, we study the interdependencies of Lyα morphological qu…

2022 Astronomy and Astrophysics
eHST 13
The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets
DOI: 10.3847/1538-3881/ac3a06 Bibcode: 2022AJ....163..128W

Cunha, Katia; Smith, Verne V.; Mahadevan, Suvrath +15 more

The chemical abundances of planet-hosting stars offer a glimpse into the composition of planet-forming environments. To further understand this connection, we make the first ever measurement of the correlation between planet occurrence and chemical abundances for ten different elements (C, Mg, Al, Si, S, K, Ca, Mn, Fe, and Ni). Leveraging data fro…

2022 The Astronomical Journal
Gaia 13
MARS: A New Maximum-entropy-regularized Strong Lensing Mass Reconstruction Method
DOI: 10.3847/1538-4357/ac69df Bibcode: 2022ApJ...931..127C

Jee, M. James; Cha, Sangjun

Free-form strong-lensing (SL) mass reconstructions typically suffer from overfitting, which manifests itself as false-positive small-scale fluctuations. We present a new free-form MAximum-entropy ReconStruction (MARS) method without the assumption that light traces mass (LTM). The MARS algorithm enables us to achieve excellent convergence in sourc…

2022 The Astrophysical Journal
eHST 13
The Nascent Milliquasar VT J154843.06+220812.6: Tidal Disruption Event or Extreme Accretion State Change?
DOI: 10.3847/1538-4357/ac5e29 Bibcode: 2022ApJ...929..184S

Hallinan, Gregg; Graham, Matthew; Lu, Wenbin +5 more

We present a detailed multiwavelength follow-up of the nuclear radio flare VT J154843.06+220812.6, hereafter VT J1548. VT J1548 was selected as a ~1 mJy radio flare in 3 GHz observations from the Very Large Array Sky Survey. It is located in the nucleus of a low-mass ( $\mathrm{log}{M}_{\mathrm{BH}}/{M}_{\odot }\sim 6$ ) host galaxy with weak or n…

2022 The Astrophysical Journal
XMM-Newton 13