Search Publications

Black Hole Spin Measurements in LMC X-1 and Cyg X-1 Are Highly Model Dependent
DOI: 10.3847/1538-4357/ad1b60 Bibcode: 2024ApJ...962..101Z

Zdziarski, Andrzej A.; Szanecki, Michał; Dewangan, Gulab +4 more

The black hole spin parameter, a *, was measured to be close to its maximum value of 1 in many accreting X-ray binaries. In particular, a * ≳ 0.9 was found in a number of studies of LMC X-1. These measurements were claimed to take into account both statistical and systematic uncertainties. We perform new measurements using a …

2024 The Astrophysical Journal
Suzaku 17
To be, or not to be: Balmer breaks in high-z galaxies with JWST
DOI: 10.1093/mnras/stae323 Bibcode: 2024MNRAS.529.1299V

Coe, Dan; Bradley, Larry D.; Zackrisson, Erik +7 more

Standard models of structure formation allow us to predict the cosmic timescales relevant for the onset of star formation and the assembly history of galaxies at high redshifts (z > 10). The strength of the Balmer break represents a well-known diagnostic of the age and star formation history of galaxies, which enables us to compare observations…

2024 Monthly Notices of the Royal Astronomical Society
JWST 17
A Comprehensive Correction of the Gaia DR3 XP Spectra
DOI: 10.3847/1538-4365/ad18b1 Bibcode: 2024ApJS..271...13H

Xiang, Maosheng; Huang, Yang; Niu, Zexi +7 more

By combining spectra from the CALSPEC and NGSL, as well as spectroscopic data from the LAMOST Data Release 7 (DR7), we have analyzed and corrected the systematic errors of the Gaia DR3 BP/RP (XP) spectra. The errors depend on the normalized spectral energy distribution (simplified by two independent "colors") and G magnitude. Our corrections are a…

2024 The Astrophysical Journal Supplement Series
Gaia eHST 17
2D disc modelling of the JWST line spectrum of EX Lupi
DOI: 10.1051/0004-6361/202347730 Bibcode: 2024A&A...683A.219W

Woitke, P.; Kamp, I.; Ábrahám, P. +3 more

We introduce a number of improvements to the thermo-chemical disc modelling code PRODIMO and new theoretical approaches that can be used to better predict and analyse the JWST line spectra of protoplanetary discs. We developed a new line escape probability method for disc geometries, and a new scheme for dust settling, and discuss how to apply UV …

2024 Astronomy and Astrophysics
Herschel XMM-Newton 17
AGNs in massive galaxy clusters: Role of galaxy merging, infalling groups, cluster mass, and dynamical state
DOI: 10.1051/0004-6361/202348212 Bibcode: 2024A&A...684A.111K

Koulouridis, E.; Drigga, E.; Gkini, A.

Context. There is compelling evidence that active galactic nuclei (AGNs) in high-density regions have undergone a different evolution than their counterparts in the field, indicating that they are strongly affected by their environment. However, we still lack a comprehensive understanding of the dominant mechanisms that trigger the nucleus and the…

2024 Astronomy and Astrophysics
XMM-Newton eHST 17
Anatomy of an ionized bubble: NIRCam grism spectroscopy of the z = 6.6 double-peaked Lyman-α emitter COLA1 and its environment
DOI: 10.1051/0004-6361/202450318 Bibcode: 2024A&A...689A..44T

Conroy, Charlie; Sobral, David; Tacchella, Sandro +10 more

The increasingly neutral intergalactic gas at z > 6 impacts the Lyman-α (Lyα) flux observed from galaxies. One luminous galaxy, COLA1, stands out because of its unique double-peaked Lyα line at z = 6.6, unseen in any simulation of reionization. Here, we present JWST/NIRCam wide-field slitless spectroscopy in a 21 arcmin2 field center…

2024 Astronomy and Astrophysics
JWST 17
SMILES: A Prototype JWST Multiband Mid-infrared Survey
DOI: 10.3847/1538-4357/ad6cd2 Bibcode: 2024ApJ...975...83R

Shivaei, Irene; Lyu, Jianwei; Alberts, Stacey +4 more

The Mid-Infrared Instrument (MIRI) for JWST is supplied with a suite of imaging band-pass filters optimized for full spectral coverage in eight intermediate-width bands from 5 to 26 µm and a narrower one at 11.3 µm. This contrasts with previous infrared space telescopes, which generally have provided only two broad bands, one near 10 &…

2024 The Astrophysical Journal
ISO 17
Chemistry of Complex Organic Molecules in the V883 Ori Disk Revealed by ALMA Band 3 Observations
DOI: 10.3847/1538-3881/ad11d9 Bibcode: 2024AJ....167...66Y

Aikawa, Yuri; Nomura, Hideko; Yamato, Yoshihide +3 more

Complex organic molecules (COMs) in protoplanetary disks are key to understanding the origin of volatiles in comets in our solar system, yet the chemistry of COMs in protoplanetary disks remains poorly understood. Here, we present Atacama Large Millimeter/submillimeter Array Band 3 observations of the disk around the young outbursting star V883 Or…

2024 The Astronomical Journal
Rosetta 17
Hunting for complex cyanides in protostellar ices with the JWST. A tentative detection of CH3CN and C2H5CN
DOI: 10.1051/0004-6361/202348695 Bibcode: 2024A&A...686A..71N

Manoj, P.; van Dishoeck, E. F.; Nazari, P. +20 more

Nitrogen-bearing complex organic molecules have been commonly detected in the gas phase but not yet in interstellar ices. This has led to the long-standing question of whether these molecules form in the gas phase or in ices. The James Webb Space Telescope (JWST) offers the sensitivity, spectral resolution, and wavelength coverage needed to detect…

2024 Astronomy and Astrophysics
JWST 17
Metal-poor stars with disc-like orbits. Possible traces of the Galactic disc at very early epochs
DOI: 10.1051/0004-6361/202348106 Bibcode: 2024A&A...683A.136B

Massari, D.; De Angeli, F.; Riello, M. +5 more

We used photometric metallicity estimates for about 700 000 stars in the surroundings of the Sun, with very accurate distances and 3D motions measures from Gaia DR3, to explore the properties of the metal-poor (−2.0 < [Fe/H] ≤ −1.5; MP) and very metal-poor ([Fe/H] ≤ −2.0; VMP) stars with disc kinematics in the sample. We confirm the presence of…

2024 Astronomy and Astrophysics
Gaia 17