Search Publications

Ubiquitous radio emission in quasars: Predominant AGN origin and a connection to jets, dust, and winds
DOI: 10.1051/0004-6361/202348982 Bibcode: 2024A&A...691A.191C

Prandoni, I.; Alexander, D. M.; Hardcastle, M. J. +16 more

We present a comprehensive study of the physical origin of radio emission in optical quasars at redshifts z < 2.5. We focus particularly on the associations between compact radio emission, dust reddening, and outflows identified in our earlier work. Leveraging the deepest low-frequency radio data available to date (LoTSS Deep DR1), we achieve r…

2024 Astronomy and Astrophysics
Herschel 16
JWST Reveals a Luminous Infrared Source at the Position of the Failed Supernova Candidate N6946-BH1
DOI: 10.3847/1538-4357/ad21fa Bibcode: 2024ApJ...964..171B

Smith, Nathan; Sand, David J.; Jencson, Jacob E. +4 more

N6946-BH1 (BH1) is the first plausible candidate for a failed supernova (SN), a peculiar event in which a massive star disappears without the expected bright SN, accompanied by collapse into a black hole (BH). Following a luminous outburst in 2009, the source experienced a significant decline in optical brightness, while maintaining a persistent I…

2024 The Astrophysical Journal
JWST 16
The black hole low-mass X-ray binary V404 Cygni is part of a wide triple
DOI: 10.1038/s41586-024-08120-6 Bibcode: 2024Natur.635..316B

Vanderburg, Andrew; Chakrabarty, Deepto; El-Badry, Kareem +7 more

Evidence suggests that, when compact objects such as black holes and neutron stars form, they may receive a 'natal kick', during which the stellar remnant gains momentum. Observational evidence for neutron star kicks is substantial1,2, yet is limited for black hole natal kicks, and some proposed black hole formation scenarios result in …

2024 Nature
eHST 16
Balmer Decrement Anomalies in Galaxies at z ∼ 6 Found by JWST Observations: Density-bounded Nebulae or Excited H I Clouds?
DOI: 10.3847/1538-4357/ad7097 Bibcode: 2024ApJ...974..180Y

Ono, Yoshiaki; Ouchi, Masami; Nakagawa, Takao +11 more

We investigate the physical origins of the Balmer decrement anomalies in GS-NDG-9422 and RXCJ2248-ID galaxies at z ∼ 6 whose Hα/Hβ values are significantly smaller than 2.7, the latter of which also shows anomalous Hγ/Hβ and Hδ/Hβ values beyond the errors. Because the anomalous Balmer decrements are not reproduced under the Case B recombination, w…

2024 The Astrophysical Journal
JWST 16
A portrait of the vast polar structure as a young phenomenon: Hints from its member satellites
DOI: 10.1051/0004-6361/202347473 Bibcode: 2024A&A...681A..73T

Steinmetz, M.; Taibi, S.; Khoperskov, S. +2 more

Context. It has been observed that several Milky Way (MW) satellite dwarf galaxies are distributed along a coherent planar distribution known as the vast polar structure (VPOS).
Aims: Here we investigate whether MW satellites located on the VPOS have different physical and orbital properties from those not associated with it.
Methods: Us…

2024 Astronomy and Astrophysics
Gaia 16
A dusty streamer infalling onto the disk of a class I protostar. ALMA dual-band constraints on grain properties and the mass-infall rate
DOI: 10.1051/0004-6361/202347486 Bibcode: 2024A&A...682A..61C

Testi, L.; Klessen, R. S.; Manara, C. F. +15 more

Context. Observations of interstellar material infalling onto star- and planet-forming systems have become increasingly common thanks to recent advancements in radio interferometry. These structures have the potential to alter the dynamics of protoplanetary disks significantly by triggering the formation of substructures, inducing shocks, and modi…

2024 Astronomy and Astrophysics
Gaia 16
Cosmic Vine: A z = 3.44 large-scale structure hosting massive quiescent galaxies
DOI: 10.1051/0004-6361/202348540 Bibcode: 2024A&A...683L...4J

Brammer, Gabriel; Greve, Thomas R.; Gillman, Steven +15 more

We report the discovery of a large-scale structure at z = 3.44 revealed by JWST data in the Extended Groth Strip (EGS) field. This structure, called the Cosmic Vine, consists of 20 galaxies with spectroscopic redshifts at 3.43 < z < 3.45 and six galaxy overdensities (4 − 7σ) with consistent photometric redshifts, making up a vine-like struct…

2024 Astronomy and Astrophysics
Gaia Herschel eHST JWST 16
Modeling the High-energy Ionizing Output from Simple Stellar and X-Ray Binary Populations
DOI: 10.3847/1538-4357/ad0a6a Bibcode: 2024ApJ...960...13G

Johnson, Benjamin D.; Tzanavaris, Panayiotis; Jaskot, Anne +9 more

We present a methodology for modeling the joint ionizing impact due to a "simple X-ray population" (SXP) and its corresponding simple stellar population (SSP), where "simple" refers to a single age and metallicity population. We construct composite spectral energy distributions (SEDs) including contributions from ultraluminous X-ray sources and st…

2024 The Astrophysical Journal
eHST 16
JWST Imaging of Edge-on Protoplanetary Disks. II. Appearance of Edge-on Disks with a Tilted Inner Region: Case Study of IRAS04302+2247
DOI: 10.3847/1538-4357/ad0c4b Bibcode: 2024ApJ...961...95V

Duchêne, Gaspard; Wolff, Schuyler G.; Perrin, Marshall D. +6 more

We present James Webb Space Telescope imaging from 2 to 21 µm of the edge-on protoplanetary disk around the embedded young star IRAS04302+2247. The structure of the source shows two reflection nebulae separated by a dark lane. The source extent is dominated by the extended filamentary envelope at ~4.4 µm and shorter wavelengths, transi…

2024 The Astrophysical Journal
Gaia eHST JWST 16
Kinematics and dynamics of the Galactic bar revealed by Gaia long-period variables
DOI: 10.1093/mnras/stae2023 Bibcode: 2024MNRAS.533.3395Z

Belokurov, Vasily; Zhang, Hanyuan; Evans, N. Wyn +2 more

We use low-amplitude long period variable (LA-LPV) candidates in Gaia DR3 to trace the kinematics and dynamics of the Milky Way bar. LA-LPVs, like other LPVs, are intrinsically bright and follow a tight period-luminosity relation, but unlike e.g. Mira variables, their radial velocity measurements are reliable due to their smaller pulsation amplitu…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 16