Search Publications

Around the Spindle Galaxy: The Dark Halo Mass of NGC 3115
DOI: 10.3847/1538-3881/ac5ab5 Bibcode: 2022AJ....163..234K

Karachentsev, I. D.; Anand, G. S.; Makarova, L. N. +1 more

We report observations of five dwarf galaxies in the vicinity of the luminous S0 galaxy NGC 3115 performed with the Advanced Camera for Surveys on the Hubble Space Telescope. Their distances determined via the Tip of the Red Giant Branch are: 10.05 Mpc (UGCA 193), 9.95 Mpc (KKSG 17), 10.13 Mpc (2MASX-J0957-0915), 10.42 Mpc (2dFGRS-TGN218Z179), and…

2022 The Astronomical Journal
eHST 8
Searching for the next Galactic Luminous red nova
DOI: 10.1093/mnras/stac2685 Bibcode: 2022MNRAS.517.1884A

Jones, David; Blagorodnova, Nadejda; Erasmus, Nicolas +3 more

Luminous red novae (LRNe) are astrophysical transients believed to be caused by the partial ejection of a binary star's common envelope (CE) and the merger of its components. The formation of the CE is likely to occur during unstable mass transfer, initiated by a primary star which is evolving off the main sequence (a Hertzsprung gap star) and a l…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
Recurrent X-ray flares of the black hole candidate in the globular cluster RZ 2109 in NGC 4472
DOI: 10.1051/0004-6361/202142662 Bibcode: 2022A&A...661A..68T

Lodato, G.; Salvaterra, R.; Tiengo, A. +7 more

We report the systematic analysis of the X-ray observations of the ultraluminous X-ray source XMMU J122939.7+075333 located in the globular cluster RZ 2109 in the Virgo galaxy NGC 4472. The inclusion of observations and time intervals ignored in previous works and the careful selection of ex…

2022 Astronomy and Astrophysics
XMM-Newton 8
Rapidly rotating stars and their transiting planets: KELT-17b, KELT-19Ab, and KELT-21b in the CHEOPS and TESS era
DOI: 10.1093/mnras/stac1095 Bibcode: 2022MNRAS.513.2822G

Kovács, J.; Claret, A.; Kundra, E. +4 more

Rapidly rotating early-type main-sequence stars with transiting planets are interesting in many aspects. Unfortunately, several astrophysical effects in such systems are not well understood yet. Therefore, we performed a photometric mini-survey of three rapidly rotating stars with transiting planets, namely KELT-17b, KELT-19Ab, and KELT-21b, using…

2022 Monthly Notices of the Royal Astronomical Society
CHEOPS Gaia 8
Stars in the local galactic thick disc and halo in Gaia EDR3: a catalogue of half a million local main-sequence stars with photometric metallicities
DOI: 10.1093/mnras/stab3671 Bibcode: 2022MNRAS.510.4308K

Kim, Bokyoung; Lépine, Sebastien

We present a catalogue of 551 214 main-sequence stars in the local (d < 2 kpc) Galactic thick disc and halo, based on a search of stars with large proper motions ($\mu _{\rm tot} \gt 40.0~\rm mas\, yr^{-1}$) in the Gaia Early Data Release 3. We derive photometric metallicity calibrated from the colour-luminosity-metallicity distribution of 20 0…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 8
FSR 1776: A new globular cluster in the Galactic bulge?
DOI: 10.1051/0004-6361/202141580 Bibcode: 2022A&A...657A..67D

Minniti, D.; Saito, R. K.; Fernández-Trincado, J. G. +6 more

Context. Recent near-IR surveys have uncovered a plethora of new globular cluster (GC) candidates towards the Milky Way bulge. These new candidates need to be confirmed as real GCs and properly characterised.
Aims: We investigate the physical nature of FSR 1776, a very interesting star cluster projected towards the Galactic bulge. This object…

2022 Astronomy and Astrophysics
Gaia 8
Interstellar objects
DOI: 10.1080/00107514.2023.2203976 Bibcode: 2022ConPh..63..200S

Moro-Martín, Amaya; Seligman, Darryl Z.

Since 2017, two macroscopic interstellar objects have been discovered in the inner Solar System, both of which are distinct in nature. The first interstellar object, 1I/`Oumuamua, passed within $\sim63$ lunar distances of the Earth, appeared asteroidal lacking detectable levels of gas or dust loss, yet exhibited a nongravitational acceleration. 1I…

2022 Contemporary Physics
Gaia 8
The non-thermal emission from the colliding-wind binary Apep
DOI: 10.1017/pasa.2021.60 Bibcode: 2022PASA...39....4D

del Palacio, S.; De Becker, M.; Romero, G. E. +2 more

Therecently discovered massive binary system Apep is the most powerful synchrotron emitter among the known Galactic colliding-wind binaries. This makes this particular system of great interest to investigate stellar winds and the non-thermal processes associated with their shocks. This source was detected at various radio bands, and in addition th…

2022 Publications of the Astronomical Society of Australia
XMM-Newton 8
The XMM Cluster Survey: an independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies
DOI: 10.1093/mnras/stac2463 Bibcode: 2022MNRAS.517..657T

Romer, A. K.; Mann, R. G.; Klein, M. +10 more

We present the first comparison between properties of clusters of galaxies detected by the eROSITA Final Equatorial-Depth Survey (eFEDS) and the XMM Cluster Survey (XCS). We have compared, in an ensemble fashion, properties from the eFEDS X-ray cluster catalogue with those from the Ultimate XMM eXtragaLactic (XXL) survey project (XXL-100-GC). We f…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 8
2D and Slab Turbulent Cascade Rates in the Inner Heliosphere
DOI: 10.3847/1538-4357/ac9234 Bibcode: 2022ApJ...938..120A

Zank, G. P.; Zhao, L. -L.; Telloni, D. +1 more

We present a theoretical and observational study of 2D and slab turbulence cascade (or heating) rates of transverse total turbulence energies, transverse cross helicity, transverse outward and inward Elsässer energy, transverse fluctuating magnetic energy density, and transverse fluctuating kinetic energy from the perihelion of the first Parker So…

2022 The Astrophysical Journal
SolarOrbiter 8