Search Publications

Improved Model of X-Ray Emission from Hot Accretion Flows
DOI: 10.3847/1538-4357/ac6c8b Bibcode: 2022ApJ...931..167N

Zdziarski, Andrzej A.; Szanecki, Michał; Niedźwiecki, Andrzej +1 more

We have developed an improved model of X-ray emission from optically thin, two-temperature accretion flows, kerrflow, using an exact Monte Carlo treatment of global Comptonization as well as with a fully general relativistic description of both the radiative and hydrodynamic processes. It also includes pion-decay electrons, whose synchrotron emiss…

2022 The Astrophysical Journal
INTEGRAL 2
Molecular Clouds Associated with H II Regions and Candidates within l = 106.°65 to 109.°50 and b = -1.°85 to 0.°95
DOI: 10.1088/1674-4527/ac52a0 Bibcode: 2022RAA....22d5008L

Zheng, Yu-Qing; Wang, Hong-Chi; Ma, Yue-Hui +3 more

We present a large-scale simultaneous survey of the CO isotopologues (12CO, 13CO, and C18O) J = 1-0 line emission toward the Galactic plane region of l = 106.°65 to 109.°50 and b = -1.°85 to 0.°95 using the Purple Mountain Observatory 13.7 m millimeter-wavelength telescope. Except for the molecular gas in the solar…

2022 Research in Astronomy and Astrophysics
Gaia 2
Catching the Butterfly and the Homunculus of η Carinae with ALMA
DOI: 10.3847/1538-4357/ac7461 Bibcode: 2022ApJ...935...76Z

Gull, Theodore R.; Menten, Karl M.; Toalá, Jesús A. +7 more

The nature and origin of the molecular gas component located in the circumstellar vicinity of η Carinae are still far from being completely understood. Here, we present Atacama Large Millimeter/submillimeter Array CO(3-2) observations with a high angular resolution (~0.″15) and a great sensitivity that are employed to reveal the origin of this com…

2022 The Astrophysical Journal
eHST 2
Estimating the Injection Duration of 20 MeV Protons in Large Western Solar Energetic Particle Events
DOI: 10.3847/1538-4357/ac609c Bibcode: 2022ApJ...930...51L

Lugaz, Noé; Li, Gen

An ad hoc analytical calculation is presented to infer the duration of injection of 20 MeV protons in 21 selected western solar energetic particle (SEP) events. We convolve the solution of diffusion equation with a "triangle" source to model the time-intensity profiles over the onset and the peaking phase. The effects of "corotating" flux tubes an…

2022 The Astrophysical Journal
SOHO 2
X-ray irradiation of three planets around Hyades star K2 -136
DOI: 10.1002/asna.20210076 Bibcode: 2022AN....34310076F

Fernández Fernández, Jorge; Wheatley, Peter J.

We study the X-ray irradiation and likely photoevaporation of the three planets around the star K2-136. These are the Earth-sized K2-136 b, the mini-Neptune K2-136 c, and the super-Earth K2-136 d. XMM-Newton observations of the star indicate an X-ray luminosity of $(1.18\pm0.1)\times10^{28}$ erg s$^{-1}$ in the range 0.15 to 2.4 keV, resulting in …

2022 Astronomische Nachrichten
Gaia XMM-Newton 2
Modeling the Photometric Variability of Alpha2 CVn with a Dynamical Magnetosphere
DOI: 10.3847/1538-4357/ac82b9 Bibcode: 2022ApJ...935..145P

Pfeffer, Cameron M.; McSwain, M. Virginia

Alpha2 Canum Venaticorum (α 2 CVn) is a strongly magnetic star with peculiar chemical signatures and periodic variability that have been long attributed to the diffusion of magnetic elements through the photosphere, leading to chemical spots across the stellar surface. However, recent studies of other magnetic hot stars are c…

2022 The Astrophysical Journal
IUE 2
Efficient labelling of solar flux evolution videos by a deep learning model
DOI: 10.1038/s41550-022-01701-3 Bibcode: 2022NatAs...6..796C

Chatterjee, Subhamoy; Muñoz-Jaramillo, Andrés; Lamb, Derek A.

Machine learning is becoming a critical tool for the interrogation of large, complex data. Labelling, defined as the process of adding meaningful annotations, is a crucial step of supervised machine learning. However, labelling datasets is time consuming. Here we show that convolutional neural networks (CNNs) trained on crudely labelled astronomic…

2022 Nature Astronomy
SOHO 2
A detailed study of the barium central star of the planetary nebula Abell 70
DOI: 10.1093/mnras/stac2501 Bibcode: 2022MNRAS.516.4833J

Munday, James; Jones, David; Miszalski, Brent +4 more

We present a detailed study of the barium star at the heart of the planetary nebula Abell 70. Time-series photometry obtained over a period of more than 10 yr demonstrates that the barium-contaminated companion is a rapid rotator with temporal variability due to spots. The amplitude and phasing of the photometric variability change abruptly; howev…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 2
Periodic Oscillations in LASCO Coronal Mass Ejection Speeds: Space Seismology
DOI: 10.3847/2041-8213/ac54b0 Bibcode: 2022ApJ...927L..16M

Gopalswamy, Nat; Yashiro, Seiji; Michalek, Grzegorz

Coronal mass ejections (CMEs) are energetic eruptions of organized magnetic structures from the Sun. Therefore, the reconnection of the magnetic field during ejection can excite periodic speed oscillations of CMEs. A previous study showed that speed oscillations are frequently associated with CME propagation. The Solar and Heliospheric Observatory…

2022 The Astrophysical Journal
SOHO 2
Morphological and hydrological analysis of volcanic flank valleys - Evidence for a volcanic origin
DOI: 10.1016/j.pss.2022.105592 Bibcode: 2022P&SS..22305592B

Bahia, Rickbir S.

Valley networks incising the flanks of Martian volcanoes are potential evidence of geologically recent fluvial activity, either via geothermal heating of snowmelt and groundwater upwelling [Gulick and Baker, 1989, 1990; Gulick et al., 1997; Gulick, 2001; Hynek et al., 2010], or summit snowpack melt [Fassett and Head, 2006, 2007]; however, their or…

2022 Planetary and Space Science
MEx 2