Search Publications

Evidence for Parametric Decay Instability in the Lower Solar Atmosphere
DOI: 10.3847/1538-4357/ac7147 Bibcode: 2022ApJ...933...52H

Hahn, Michael; Fu, Xiangrong; Savin, Daniel Wolf

We find evidence for the first observation of the parametric decay instability (PDI) in the lower solar atmosphere. In particular, we find that the power spectrum of density fluctuations near the solar transition region resembles the power spectrum of the velocity fluctuations but with the frequency axis scaled up by about a factor of 2. These res…

2022 The Astrophysical Journal
IRIS 8
Analysis of multiscale structures at the quasi-perpendicular Venus bow shock. Results from Solar Orbiter's first Venus flyby
DOI: 10.1051/0004-6361/202140954 Bibcode: 2022A&A...660A..64D

Maksimovic, M.; Bale, S. D.; Chust, T. +23 more

Context. Solar Orbiter is a European Space Agency mission with a suite of in situ and remote sensing instruments to investigate the physical processes across the inner heliosphere. During the mission, the spacecraft is expected to perform multiple Venus gravity assist maneuvers while providing measurements of the Venusian plasma environment. The f…

2022 Astronomy and Astrophysics
SolarOrbiter 8
Seimei KOOLS-IFU mapping of the gas and dust distributions in Galactic planetary nebulae: the case of IC 2165
DOI: 10.1093/mnras/stac260 Bibcode: 2022MNRAS.511.4774O

Otsuka, Masaaki

We investigated the physical and chemical properties of the gas and dust components in a carbon-rich planetary nebula (PN) IC 2165 using two-dimensional emission-line maps with superior resolution. The extinction map is generated in a self-consistent and assumption-free manner. The circumstellar gas-to-dust mass ratio (GDR) map ranges radially fro…

2022 Monthly Notices of the Royal Astronomical Society
AKARI IUE eHST 8
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