Search Publications

The Milky Way Bulge Extra-tidal Star Survey: BH 261 (AL 3)
DOI: 10.3847/1538-3881/ad0cfc Bibcode: 2024AJ....167...21K

Clarkson, William I.; Kunder, Andrea; Johnson, Christian I. +19 more

The Milky Way Bulge extra-tidal star survey is a spectroscopic survey with the goal of identifying stripped globular cluster stars from inner Galaxy clusters. In this way, an indication of the fraction of metal-poor bulge stars that originated from globular clusters can be determined. We observed and analyzed stars in and around BH 261, an underst…

2024 The Astronomical Journal
Gaia 2
The mass distribution of stellar mergers: A new scenario for several FS CMa stars
DOI: 10.1051/0004-6361/202449586 Bibcode: 2024A&A...689A.234D

Korčáková, D.; Kroupa, P.; Dvořáková, N. +1 more

Context. FS CMa stars belong to a diverse group of stars exhibiting the B[e] phenomenon, which manifests itself mainly by the presence of forbidden emission lines and a strong infrared (IR) excess in their spectra. Only a few tens of FS CMa stars are known and their nature is still unclear. Recently, a strong magnetic field has been discovered in …

2024 Astronomy and Astrophysics
Gaia 2
Cygnus A obscuring torus: ionized, atomic, or molecular?
DOI: 10.1093/mnras/stad3328 Bibcode: 2024MNRAS.527.2371B

Ogle, Patrick; Antonucci, Robert; Bagul, Atharva +2 more

The prototypical powerful FR II radio galaxy Cygnus A fits extremely well into the quasar/radio galaxy unified model: high polarization with an angle almost perpendicular to the radio jet and polarized flux showing broad permitted lines. It has been claimed that ionized gas in the torus reveals a very clear torus shape via Bremmstrahlung emission.…

2024 Monthly Notices of the Royal Astronomical Society
Herschel 2
The MUSE Ultra Deep Field (MUDF). VI. The Relationship between Galaxy Properties and Metals in the Circumgalactic Medium
DOI: 10.3847/1538-4357/ad702d Bibcode: 2024ApJ...974..256B

Rafelski, Marc; Beckett, Alexander; Fumagalli, Michele +10 more

We present initial results associating galaxies in the Multi-Unit Spectroscopic Explorer (MUSE) Ultra Deep Field (MUDF) with gas seen in absorption along the line of sight to two bright quasars in this field to explore the dependence of metals in the circumgalactic medium (CGM) on galaxy properties. The MUDF includes ∼140 hr of Very Large Telescop…

2024 The Astrophysical Journal
eHST 2
Discovery of a new IW And-type dwarf nova with both tilted disc and tidal instability
DOI: 10.1093/mnras/stae1025 Bibcode: 2024MNRAS.531..422S

Shi, Jianrong; Huang, Yang; Liu, Jifeng +6 more

IW And-type dwarf novae are anomalous Z Cam stars featured with outbursts happening during standstill states, which are not expected in the standard disc instability model. The physical mechanisms for these variations remain unclear. In this study, we report the discovery of a new candidate IW And-type dwarf nova J0652+2436, identified with its fr…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 2
On the mass assembly history of the Milky Way: clues from its stellar halo
DOI: 10.1007/s10509-024-04370-y Bibcode: 2024Ap&SS.369..107H

Horta, Danny; Schiavon, Ricardo P.

Stellar halos of galaxies retain crucial clues to their mass assembly history. It is in these galactic components that the remains of cannibalised galactic building blocks are deposited. For the case of the Milky Way, the opportunity to analyse the stellar halo's structure on a star-by-star basis in a multi-faceted approach provides a basis from w…

2024 Astrophysics and Space Science
Gaia 2
Detection of the neutral iron line from the supernova remnant W 49 B with Suzaku
DOI: 10.1093/pasj/psae006 Bibcode: 2024PASJ...76..265S

Katsuda, Satoru; Nobukawa, Masayoshi; Nobukawa, Kumiko K. +2 more

Recent studies of supernova remnants (SNRs) have revealed that some SNRs exhibit a neutral iron line emission at 6.4 keV. This line has been proposed to originate from the interaction of high-energy particles formed in the SNR shell with the surrounding cold matter. We searched for the neutral iron line emission in the SNR W 49 B. Significant dete…

2024 Publications of the Astronomical Society of Japan
Suzaku 2
Modeling of the Polytropic Index and Temperature Anisotropy in the Solar Wind
DOI: 10.3847/1538-4357/ad380e Bibcode: 2024ApJ...966..142D

Engelbrecht, N. E.; Strauss, R. D.; Desta, Ephrem Tesfaye

The polytropic index is a fundamental physical parameter related to the thermodynamic processes present in space and astrophysical plasmas. This paper investigates the theoretical relationship between the polytropic index and the temperature anisotropy for flow parameters relevant to space plasmas. The derivation is based on the Chew–Goldberger–Lo…

2024 The Astrophysical Journal
Ulysses 2
Magnetic Fields in Giant Filaments Probed by the Velocity Gradient Technique: Regular Magnetic Field Interrupted by Magnetization Gaps
DOI: 10.3847/1538-4357/ad09df Bibcode: 2024ApJ...961..124Z

Li, Dalei; Tang, Xindi; Zhou, Jianjun +7 more

We study the magnetic field structures in six giant filaments associated with the spiral arms of the Milky Way by applying the velocity gradient technique (VGT) to the 13CO spectroscopic data from the GRS, FUGIN, and SEDIGSM surveys. Unlike dust-polarized emission, the VGT allows us to separate the foreground and background using the ve…

2024 The Astrophysical Journal
Herschel 2
Comets, sliding of surface dust on illuminated surfaces
DOI: 10.1016/j.icarus.2023.115861 Bibcode: 2024Icar..41015861K

Kossacki, Konrad J.; Wesołowski, Marcin; Mikołajków, Tomasz +1 more

In our paper we presented the results of our laboratory experiments dealing with the formation and sliding of the desiccated nonvolatile granular material down the samples of potential cometary analogs. The studied samples were composed of porous aggregates containing water ice, quartz sand and charcoal. Their surfaces were initially free of desic…

2024 Icarus
Rosetta 2