Search Publications

The Astrometric Animation of Water Masers toward the Mira Variable BX Cam
DOI: 10.3847/1538-4357/ac9599 Bibcode: 2022ApJ...941..105X

Kim, Dong-Jin; Sun, Yan; Orosz, Gabor +20 more

We report very long baseline interferometry (VLBI) monitoring observations of the 22 GHz water (H2O) masers around the Mira variable BX Cam, which were carried out as a part of the EAVN Synthesis of Stellar Maser Animations project. Data of 37 epochs in total were obtained from 2018 May to 2021 June with a time interval of 3-4 weeks, sp…

2022 The Astrophysical Journal
Gaia 6
Catalogue of stars measured in the Geneva seven-colour photometric system
DOI: 10.1051/0004-6361/202142355 Bibcode: 2022A&A...661A..89P

Paunzen, E.

Context. The Geneva seven-colour photometric system is successfully applied to the study of various astrophysical objects. It measures the slope of the Paschen continuum, the Balmer discontinuity, and blocking absorption due to hydrogen or metallic lines. One of its greatest strengths is its intrinsic homogeneity.
Aims: A new catalogue of the…

2022 Astronomy and Astrophysics
Gaia 6
Dust emissivity in resolved spiral galaxies
DOI: 10.1051/0004-6361/202243930 Bibcode: 2022A&A...664A.187B

Clark, Christopher J. R.; De Looze, Ilse; Baes, Maarten +12 more

Context. The far-infrared (FIR) and sub-millimeter (submm) emissivity, ϵν, of the Milky Way (MW) cirrus is an important benchmark for dust grain models. Dust masses in other galaxies are generally derived from the FIR/submm using the emission properties of these MW-calibrated models.
Aims: We seek to derive the FIR/submm ϵν

2022 Astronomy and Astrophysics
Herschel 6
L-GALAXIES 2020: the formation and chemical evolution of stellar haloes in Milky Way analogues and galaxy clusters
DOI: 10.1093/mnras/stab3568 Bibcode: 2022MNRAS.510.1945M

Yates, Robert M.; Mohamed, Shazrene S.; Murphy, Geoff G.

We present an analysis of the formation and chemical evolution of stellar haloes around (a) Milky Way analogue (MWA) galaxies and (b) galaxy clusters in the L-GALAXIES 2020 semi-analytic model of galaxy evolution. Observed stellar halo properties are better reproduced when assuming a gradual stripping model for the removal of cold gas and stars fr…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 6
The binary system of the spinning-top Be star Achernar
DOI: 10.1051/0004-6361/202244009 Bibcode: 2022A&A...667A.111K

Klement, Robert; Rivinius, Thomas; Mérand, Antoine +16 more

Context. Achernar, the closest and brightest classical Be star, presents rotational flattening, gravity darkening, occasional emission lines due to a gaseous disk, and an extended polar wind. It is also a member of a close binary system with an early A-type dwarf companion.
Aims: We aim to determine the orbital parameters of the Achernar syst…

2022 Astronomy and Astrophysics
Gaia 6
An estimate of the mass of the Milky Way from the Magellanic Stream
DOI: 10.1093/mnras/stac2308 Bibcode: 2022MNRAS.517.1737C

Baum, Stefi; Chakrabarti, Sukanya; Craig, Peter A. +1 more

We present a model for the formation of the Magellanic Stream (MS) due to ram pressure stripping. We model the history of the Small and Large Magellanic Clouds in the recent cosmological past in a static Milky Way (MW) potential with diffuse halo gas, using observationally motivated orbits for the Magellanic Clouds derived from HST proper motions …

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 6
Dust scattering halo around the CCO in HESS J1731-347: A detailed analysis
DOI: 10.1051/0004-6361/202142334 Bibcode: 2022A&A...659A..82L

Pühlhofer, G.; Doroshenko, V.; Landstorfer, A.

The supernova remnant (SNR) HESS J1731−347 is one of the few objects exhibiting emission up to the TeV energy band and it stands as a prime target for the study of cosmic ray acceleration in SNRs. It also hosts a central compact object (CCO), which is of interest in the context of the ultra-dense matter equation of state in neutron stars. For both…

2022 Astronomy and Astrophysics
Gaia 6
Deep near-infrared survey towards the W40 and Serpens South region in the Aquila Rift: A comprehensive catalogue of young stellar objects
DOI: 10.1093/mnras/stac2191 Bibcode: 2022MNRAS.516.5244S

Wang, Hongchi; Gutermuth, Robert A.; Ma, Yuehui +5 more

Active star-forming regions are excellent laboratories for studying the origins and evolution of young stellar object (YSO) clustering. The W40-Serpens South region is such a region, and we compile a large near- and mid-infrared catalogue of point sources in it, based on deep near-infrared observations of Canada-France-Hawaii Telescope (CFHT) in c…

2022 Monthly Notices of the Royal Astronomical Society
Herschel 6
Sudden depletion of Alfvénic turbulence in the rarefaction region of corotating solar wind high-speed streams at 1 AU: Possible solar origin?
DOI: 10.1051/0004-6361/202040006 Bibcode: 2022A&A...661A..64C

Pietropaolo, E.; Bruno, R.; Marino, R. +2 more

A canonical description of a corotating solar wind high-speed stream in terms of velocity profile would indicate three main regions: a stream interface or corotating interaction region characterized by a rapid increase in flow speed and by compressive phenomena that are due to dynamical interaction between the fast wind flow and the slower ambient…

2022 Astronomy and Astrophysics
SolarOrbiter 6
High-latitude Observations of Inertial-range Turbulence by the Ulysses Spacecraft During the Solar Minimum of 1993-96
DOI: 10.3847/1538-4357/ac4588 Bibcode: 2022ApJ...927...43W

Isenberg, Philip A.; Schwadron, Nathan A.; Murphy, Neil +8 more

We have examined Ulysses magnetic field measurements for the years 1993 through 1996 as the spacecraft moved sunward from 5 au at high southern latitudes, passing through perihelion during the first fast-latitude scan to achieve high northern latitudes, and finally returning to 5 au. These years represent near-solar-minimum activity, providing a c…

2022 The Astrophysical Journal
Ulysses 6