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X-Ray Studies of the Pulsar PSR J1420-6048 and Its TeV Pulsar Wind Nebula in the Kookaburra Region
DOI: 10.3847/1538-4357/acb1b0 Bibcode: 2023ApJ...945...33P

Woo, Jooyun; An, Hongjun; Mori, Kaya +4 more

We present a detailed analysis of broadband X-ray observations of the pulsar PSR J1420-6048 and its wind nebula (PWN) in the Kookaburra region with Chandra, XMM-Newton, and NuSTAR. Using the archival XMM-Newton and new NuSTAR data, we detected 68 ms pulsations of the pulsar and characterized its X-ray pulse profile, which exhibits a sharp spike an…

2023 The Astrophysical Journal
XMM-Newton 6
Asteroseismic Modeling of 1153 Kepler Red Giant Branch Stars: Improved Stellar Parameters with Gravity-mode Period Spacings and Luminosity Constraints
DOI: 10.3847/1538-4357/ace4c9 Bibcode: 2023ApJ...953..182W

Bi, Shaolan; Li, Yaguang; Bedding, Timothy R. +2 more

This paper reports the estimated stellar parameters of 1153 Kepler red giant branch stars determined with asteroseismic modeling. We use radial-mode oscillation frequencies, gravity-mode period spacings, Gaia luminosities, and spectroscopic data to characterize these stars. Compared with previous studies, we find that the two additional observed c…

2023 The Astrophysical Journal
Gaia 6
HST PanCET programme: a flat optical transmission spectrum for the Hot Jupiter WASP-101b
DOI: 10.1093/mnras/stad1010 Bibcode: 2023MNRAS.522..582R

Mikal-Evans, Thomas; Sing, David K.; López-Morales, Mercedes +10 more

We present an optical transmission spectrum of the hot Jupiter WASP-101b. We observed three primary transits with Hubble Space Telescope (HST)/Space Telescope Imaging Spectrograph, covering a wavelength range from 0.3 to 1 $\mu$m. The observations suffer from significant systematics that we model using Gaussian Processes. Kernel selection for the …

2023 Monthly Notices of the Royal Astronomical Society
eHST 6
Simulating the charging of isolated free-falling masses from TeV to eV energies: Detailed comparison with LISA Pathfinder results
DOI: 10.1103/PhysRevD.107.022010 Bibcode: 2023PhRvD.107b2010W

Hollington, D.; Wass, P. J.; Sumner, T. J. +1 more

A model is presented that explains the charging rate of the LISA Pathfinder test masses by the interplanetary cosmic ray environment. The model incorporates particle-tracking from TeV to eV energies using a combination of GEANT4 and a custom low-energy particle generation and tracking code. The electrostatic environment of the test mass is simulat…

2023 Physical Review D
LISAPathfinder 6
Mid-IR spectral properties of different surfaces of silicate mixtures before and after excimer laser irradiation
DOI: 10.1016/j.icarus.2023.115683 Bibcode: 2023Icar..40415683W

Hiesinger, Harald; Helbert, Jörn; Weber, Iris +6 more

The behaviour of the Christiansen feature (CF) and the Reststrahlen bands (RBs) in mid-infrared (IR) reflectance spectra on various silicate mixtures as pressed pellets and powders was investigated in high-vacuum. In addition, the influence of micrometeorite bombardment simulated with an excimer laser was studied. The mixtures cover a wide range o…

2023 Icarus
BepiColombo 6
MagAO-X and HST High-contrast Imaging of the AS209 Disk at Hα
DOI: 10.3847/1538-3881/acf375 Bibcode: 2023AJ....166..162C

Edwards, Suzan; Zhou, Yifan; Bae, Jaehan +22 more

The detection of emission lines associated with accretion processes is a direct method for studying how and where gas giant planets form, how young planets interact with their natal protoplanetary disk, and how volatile delivery to their atmosphere takes place. Hα (λ = 0.656 µm) is expected to be the strongest accretion line observable from …

2023 The Astronomical Journal
Gaia eHST 6
A Coronal Mass Ejection Source Region Catalog and Their Associated Properties
DOI: 10.3847/1538-4365/aceb62 Bibcode: 2023ApJS..268...38M

Pant, Vaibhav; Banerjee, Dipankar; Patel, Ritesh +4 more

The primary objective of this study is to connect coronal mass ejections (CMEs) to their source regions, primarily to create a CME source region catalog, and secondarily to probe the influence that the source regions have on the different statistical properties of CMEs. We create a source region catalog for 3327 CMEs from 1998 to 2017, thus captur…

2023 The Astrophysical Journal Supplement Series
SOHO 6
Near-infrared Spectroscopy of Dense Ejecta Knots in the Outer Eastern Area of the Cassiopeia A Supernova Remnant
DOI: 10.3847/1538-4357/acda2d Bibcode: 2023ApJ...953..131K

Koo, Bon-Chul; Lee, Jae-Joon; Yoon, Sung-Chul +1 more

The Cassiopeia A supernova remnant has a complex structure, manifesting the multidimensional nature of core-collapse supernova explosions. To further understand this, we carried out near-infrared multiobject spectroscopy on the ejecta knots located in the northeastern (NE) jet and Fe K plume regions, which are two distinct features in the outer ea…

2023 The Astrophysical Journal
Herschel 6
Activity distribution of comet 67P/Churyumov-Gerasimenko from combined measurements of non-gravitational forces and torques
DOI: 10.1051/0004-6361/202245243 Bibcode: 2023A&A...670A.170A

Jorda, L.; Agarwal, J.; Groussin, O. +5 more


Aims: Understanding the activity is vital for deciphering the structure, formation, and evolution of comets. We investigate models of cometary activity by comparing them to the dynamics of 67P/Churyumov-Gerasimenko.
Methods: We matched simple thermal models of water activity to the combined Rosetta datasets by fitting to the total outgas…

2023 Astronomy and Astrophysics
Rosetta 6
Chemical abundances of the Typhon stellar stream
DOI: 10.1093/mnras/stac2757 Bibcode: 2023MNRAS.519.4467J

Ting, Yuan-Sen; Naidu, Rohan P.; Simon, Joshua D. +2 more

We present the first high-resolution chemical abundances of seven stars in the recently discovered high-energy stream Typhon. Typhon stars have apocentres r ≳ 100 kpc, making this the first detailed chemical picture of the Milky Way's very distant stellar halo. Though the sample size is limited, we find that Typhon's chemical abundances are more l…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 6