Search Publications

Magnetic Fields of the Starless Core L 1512
DOI: 10.3847/1538-4357/ad0cc1 Bibcode: 2024ApJ...961..117L

Pattle, Kate; Ward-Thompson, Derek; Berry, David +6 more

We present JCMT POL-2 850 µm dust polarization observations and Mimir H-band stellar polarization observations toward the starless core L 1512. We detect the highly ordered core-scale magnetic field traced by the POL-2 data, of which the field orientation is consistent with the parsec-scale magnetic fields traced by Planck data, suggesting t…

2024 The Astrophysical Journal
Gaia 5
The MIRI Exoplanets Orbiting White dwarfs (MEOW) Survey: Mid-infrared Excess Reveals a Giant Planet Candidate around a Nearby White Dwarf
DOI: 10.3847/2041-8213/ad74ed Bibcode: 2024ApJ...973L..11L

Vanderburg, Andrew; Stevenson, Kevin B.; MacDonald, Ryan J. +17 more

The MIRI Exoplanets Orbiting White dwarfs survey is a cycle 2 JWST program to search for exoplanets around dozens of nearby white dwarfs via infrared excess and direct imaging. In this Letter, we present the detection of mid-infrared excess at 18 and 21 µm toward the bright (V = 11.4) metal-polluted white dwarf WD 0310–688. The source of the…

2024 The Astrophysical Journal
Gaia JWST 5
First measurement of the triaxiality of the inner dark matter halo of the Milky Way
DOI: 10.1051/0004-6361/202451743 Bibcode: 2024A&A...691A.277W

Helmi, Amina; Woudenberg, Hanneke C.

Context. Stellar streams are particularly sensitive probes of the mass distribution of galaxies. Aims. In this work, we focus on the Helmi streams (HS), the remnants of an accreted dwarf galaxy orbiting the inner Milky Way. We examined their peculiar dynamical properties in depth, and used these to provide tight constraints on the Galactic potenti…

2024 Astronomy and Astrophysics
Gaia 5
Revisiting the Dragonfly galaxy II. Young, radiatively efficient radio-loud AGN drives massive molecular outflow in a starburst merger at z = 1.92
DOI: 10.1093/mnras/stae798 Bibcode: 2024MNRAS.529.4531Z

Inoue, Akio K.; Sugahara, Yuma; Kaneko, Hiroyuki +4 more

Radio-loud active galactic nuclei (RLAGNs) are a unique AGN population and were thought to be preferentially associated with supermassive black holes (SMBHs) at low accretion rates. They could impact the host galaxy evolution by expelling cold gas through the jet-mode feedback. In this work, we studied CO(6-5) line emission and continuum emission …

2024 Monthly Notices of the Royal Astronomical Society
eHST 5
Wolf 327b: A new member of the pack of ultra-short-period super-Earths around M dwarfs
DOI: 10.1051/0004-6361/202348813 Bibcode: 2024A&A...684A..83M

Nagel, E.; Amado, P. J.; Caballero, J. A. +52 more

Planets with orbital periods shorter than 1 day are rare and have formation histories that are not completely understood. Small (Rp < 2 R) ultra-short-period (USP) planets are highly irradiated, probably have rocky compositions with high bulk densities, and are often found in multi-planet systems. Additionally, USP planet…

2024 Astronomy and Astrophysics
Gaia 5
CHEX-MATE: CLUster Multi-Probes in Three Dimensions (CLUMP-3D). I. Gas analysis method using X-ray and Sunyaev-Zel'dovich effect data
DOI: 10.1051/0004-6361/202347399 Bibcode: 2024A&A...686A..97K

Lovisari, Lorenzo; Umetsu, Keiichi; Okabe, Nobuhiro +23 more

Galaxy clusters are the products of structure formation through myriad physical processes that affect their growth and evolution throughout cosmic history. As a result, the matter distribution within galaxy clusters, or their shape, is influenced by cosmology and astrophysical processes, in particular the accretion of new material due to gravity. …

2024 Astronomy and Astrophysics
Herschel XMM-Newton 5
Windy or Not: Radio Parsec-scale Evidence for a Broad-line Region Wind in Radio-quiet Quasars
DOI: 10.3847/1538-4357/ad74fc Bibcode: 2024ApJ...975...35C

Gelfand, Joseph D.; Laor, Ari; Paragi, Zsolt +6 more

Does a broad-line region (BLR) wind in radio-quiet (RQ) active galactic nuclei (AGN) extend to parsec scales and produce radio emission? We explore the correlations between a parsec-scale radio wind and the BLR wind in a sample of 19 RQ Palomar–Green quasars. The radio wind is defined based on the spectral slope and the compactness of the emission…

2024 The Astrophysical Journal
XMM-Newton 5
Shockingly Bright Warm Carbon Monoxide Molecular Features in the Supernova Remnant Cassiopeia A Revealed by JWST
DOI: 10.3847/2041-8213/ad5186 Bibcode: 2024ApJ...969L...9R

Fransson, C.; Smith, N.; Rest, A. +36 more

We present JWST NIRCam (F356W and F444W filters) and MIRI (F770W) images and NIRSpec Integral Field Unit (IFU) spectroscopy of the young Galactic supernova remnant Cassiopeia A (Cas A) to probe the physical conditions for molecular CO formation and destruction in supernova ejecta. We obtained the data as part of a JWST survey of Cas A. The NIRCam …

2024 The Astrophysical Journal
JWST 5
Supermassive Black Hole Winds in X-rays: SUBWAYS. III. A population study on ultra-fast outflows
DOI: 10.1051/0004-6361/202348908 Bibcode: 2024A&A...687A.235G

Maiolino, R.; Merloni, A.; Fiore, F. +44 more

The detection of blueshifted absorption lines likely associated with ionized iron K-shell transitions in the X-ray spectra of many active galactic nuclei (AGNs) suggests the presence of a highly ionized gas outflowing with mildly relativistic velocities (0.03c-0.6c) named ultra-fast outflow (UFO). Within the SUBWAYS project, we characterized these…

2024 Astronomy and Astrophysics
XMM-Newton 5
Observed seasonal changes in Martian hydrogen chloride explained by heterogeneous chemistry
DOI: 10.1051/0004-6361/202449546 Bibcode: 2024A&A...687A.191T

Montmessin, Franck; Trokhimovskiy, Alexander; Korablev, Oleg +7 more


Aims: The aim of this work is to show that the seasonal changes and vertical distribution profiles of hydrogen chloride (HCl) on Mars, as observed by the ExoMars Trace Gas Orbiter, are consistent with the production of gas-phase chlorine atoms from airborne dust and a subsequent rapid uptake of HCl onto water ice particles.
Methods: A 1D…

2024 Astronomy and Astrophysics
ExoMars-16 5