Search Publications

Heavy-ion Acceleration in 3He-rich Solar Energetic Particle Events: New Insights from Solar Orbiter
DOI: 10.3847/1538-4357/acf31b Bibcode: 2023ApJ...957..112M

Lario, D.; Wimmer-Schweingruber, R. F.; Allen, R. C. +7 more

We present Solar Orbiter energetic particle observations of two 3He-rich events with features more clearly observed than in prior studies. The event of 2022 November 9 observed from 0.59 au contained hundreds of ultraheavy (UH; mass >78 amu) ions whereas previous observations at 1 au have shown only an occasional count or two. The ev…

2023 The Astrophysical Journal
SolarOrbiter 10
On the evolution of the size of Lyman alpha haloes across cosmic time: no change in the circumgalactic gas distribution when probed by line emission
DOI: 10.1093/mnras/stad1264 Bibcode: 2023MNRAS.522.4275R

Blaizot, Jérémy; Garel, Thibault; Verhamme, Anne +18 more

Lyman α (Lyα) is now routinely used as a tool for studying high-redshift galaxies, and its resonant nature means it can trace neutral hydrogen around star-forming galaxies. Integral field spectrograph measurements of high-redshift Lyα emitters indicate that significant extended Lyα halo emission is ubiquitous around such objects. We present a samp…

2023 Monthly Notices of the Royal Astronomical Society
eHST 10
A fresh perspective on the 3D dynamics of Tycho's supernova remnant: Ejecta asymmetries in the X-ray band
DOI: 10.1051/0004-6361/202346954 Bibcode: 2023A&A...680A..80G

Ballet, J.; Decourchelle, A.; Acero, F. +1 more

Context. Even 450 yr after the explosion of the Type Ia SN 1572, the dynamics of the Tycho supernova remnant (Tycho's SNR) can offer keys to improving our understanding of the explosion mechanism and the interaction of the remnant with the interstellar medium.
Aims: To probe the asymmetries and the evolution of the SNR, we tracked the ejecta …

2023 Astronomy and Astrophysics
Gaia 10
HAZMAT. IX. An Analysis of the UV and X-Ray Evolution of Low-mass Stars in the Era of Gaia
DOI: 10.3847/1538-4357/acd2dc Bibcode: 2023ApJ...951...44R

Jackman, James A. G.; Peacock, Sarah; Barman, Travis +6 more

Low-mass stars (≤1 M ) are some of the best candidates for hosting planets with detectable life because of these stars' long lifetimes and relative ratios of planet to star mass and radius. An important aspect of these stars to consider is the amount of ultraviolet (UV) and X-ray radiation incident on planets in the habitable zones due…

2023 The Astrophysical Journal
Gaia 10
The ubiquity of carbon dredge-up in hydrogen-deficient white dwarfs as revealed by GALEX
DOI: 10.1093/mnrasl/slad105 Bibcode: 2023MNRAS.525L.112B

Blouin, Simon; Kilic, Mukremin; Tremblay, Pier-Emmanuel +1 more

The convective dredge-up of carbon from the interiors of hydrogen-deficient white dwarfs has long been invoked to explain the presence of carbon absorption features in the spectra of cool DQ stars ($T_{\rm eff} \lt 10\,000\,$K). It has been hypothesized that this transport process is not limited to DQ white dwarfs and also operates, albeit less ef…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 10
Revealing the structure of the lensed quasar Q 0957+561. III. Constraints on the size of the broad-line region
DOI: 10.1051/0004-6361/202140975 Bibcode: 2023A&A...678A.108F

Hanslmeier, A.; Muñoz, J. A.; Mediavilla, E. +6 more


Aims: Our aim is to examine the size, kinematics, and geometry of the broad-line region (BLR) in the double-lensed quasar Q 0957+561 by analyzing the impact of microlensing on various rest-frame ultraviolet broad-emission lines (BELs).
Methods: We explore the influence of intrinsic variability and microlensing on the C IV, C III], and Mg…

2023 Astronomy and Astrophysics
eHST 10
Dissecting the Mid-infrared Heart of M83 with JWST
DOI: 10.3847/1538-4357/acc837 Bibcode: 2023ApJ...948..124H

Kumari, Nimisha; Hirschauer, Alec S.; Hernandez, Svea +10 more

We present a first look at the MRS observations of the nucleus of the nearby galaxy M83, taken with MIRI on board JWST. The observations show a rich set of emission features from the ionized gas, warm molecular gas, and dust. To begin dissecting the complex processes in this part of the galaxy, we divide the observations into four different region…

2023 The Astrophysical Journal
ISO eHST JWST 10
Flares, Rotation, Activity Cycles, and a Magnetic Star–Planet Interaction Hypothesis for the Far-ultraviolet Emission of GJ 436
DOI: 10.3847/1538-3881/acbbc8 Bibcode: 2023AJ....165..146L

Loyd, R. O. Parke; Jackman, James A. G.; France, Kevin +6 more

Variability in the far-ultraviolet (FUV) emission produced by stellar activity affects photochemistry and heating in orbiting planetary atmospheres. We present a comprehensive analysis of the FUV variability of GJ 436, a field-age M2.5V star (P rot ≈ 44 days) that is orbited by a warm Neptune-sized planet (M ≈ 25 M , R ≈ 4.1…

2023 The Astronomical Journal
eHST 10
RELICS: A Strong-lens Model of SMACS J0723.3-7327
DOI: 10.3847/1538-4365/aca7c3 Bibcode: 2023ApJS..264...15S

Mahler, Guillaume; Coe, Dan; Sharon, Keren +2 more

We present the details of a strong-lens model of SMACS J0723.3-7327, which was made public as part of the data and high-level science products (HLSP) release of the RELICS Hubble Space Telescope (HST) treasury program (Reionization Lensing Cluster Survey; GO-14096, PI: Coe). The model products were made available on the Mikulski Archive for Space …

2023 The Astrophysical Journal Supplement Series
eHST 10
Hyades Member K2-136c: The Smallest Planet in an Open Cluster with a Precisely Measured Mass
DOI: 10.3847/1538-3881/acca1c Bibcode: 2023AJ....165..235M

Vanderburg, Andrew; Shkolnik, Evgenya; López-Morales, Mercedes +39 more

K2-136 is a late-K dwarf (0.742 ± 0.039 M ) in the Hyades open cluster with three known, transiting planets and an age of 650 ± 70 Myr. Analyzing K2 photometry, we found that planets K2-136b, c, and d have periods of 8.0, 17.3, and 25.6 days and radii of 1.014 ± 0.050 R , 3.00 ± 0.13 R , and 1.565 ± 0.077 R

2023 The Astronomical Journal
Gaia XMM-Newton eHST 10