Search Publications

Blazars at Very High Energies: Emission Modelling
DOI: 10.3390/galaxies10060105 Bibcode: 2022Galax..10..105S

Zech, Andreas; Sol, Hélène

Blazars are very broadband cosmic sources with spectra spanning over twenty orders of magnitude in frequency, down to the 100 MHz regime in the radio range, up to VHE at several tens of TeV. The modelling of their spectral energy distribution at high energies currently considers two main classes of models, leptonic and lepto-hadronic, which both s…

2022 Galaxies
Gaia 10
Fundamental Properties of Late-Type Stars in Eclipsing Binaries
DOI: 10.3390/galaxies10050098 Bibcode: 2022Galax..10...98M

Ribas, Ignasi; Giménez, Álvaro; Morales, Juan Carlos +1 more

Evidence from the analysis of eclipsing binary systems revealed that late-type stars are larger and cooler than predicted by models, and that this is probably caused by stellar magnetic activity. In this work, we revisit this problem taking into account the advancements in the last decade. We provide and updated a list of 32 eclipsing binary or mu…

2022 Galaxies
Gaia 10
A Preliminary Investigation of CSPN in the HASH Database
DOI: 10.3390/galaxies10010032 Bibcode: 2022Galax..10...32P

Parker, Quentin A.; Ritter, Andreas; Xiang, Zou

We present some preliminary findings on the population of planetary nebula where central stars (CSPN) have been independently identified in the HASH catalogue. Many new discoveries and candidates have been found (416 at the time of this writing), adding significantly to the previously known sample of about 600. We also present results from a compa…

2022 Galaxies
Gaia 7
Further Studies of the Association of Planetary Nebula BMP J16135406 with Galactic Open Cluster NGC 6067
DOI: 10.3390/galaxies10020044 Bibcode: 2022Galax..10...44F

Parker, Quentin A.; Sabin, Laurence; Zijlstra, Albert A. +3 more

Planetary Nebulae (PNe) that are physical members of Galactic open clusters are powerful probes that allow precise determination of their distance and crucially their initial mass on the main sequence. Here, we revisit the physical association of the PN BMP J1613–5406 with the open cluster NGC 6067 and present our preliminary results based on our …

2022 Galaxies
Gaia 4
The Accreting White Dwarfs in Cataclysmic Variables
DOI: 10.3390/galaxies10020043 Bibcode: 2022Galax..10...43S

Sion, Edward M.; Godon, Patrick

Accreting white dwarfs (WDs) in cataclysmic variables (CVs) provide crucial insights about the accretion of mass and angular momentum in all types of binaries, including accreting NSs and BHs. Accreting WDs are the critical component in the single degenerate pathway to SNe Ia, along with the double degenerate merger pathway, they are the standard …

2022 Galaxies
Gaia eHST 4
Millimetre Observations of Maser-Emitting Planetary Nebulae
DOI: 10.3390/galaxies10020048 Bibcode: 2022Galax..10...48U

Boumis, Panayotis; Ramos-Larios, Gerardo; Miranda, Luis F. +7 more

Observations in the millimetre bands of maser-emitting planetary nebulae (PNe) are crucial to study their circumstellar molecular gas at the beginning of the PN phase. Maser-emitting PNe are in the earliest phases of PN formation; therefore, these sources are key objects to study the molecular content during the early evolution of PNe. These circu…

2022 Galaxies
Gaia 1