Search Publications

VLT/X-shooter spectroscopy of massive young stellar objects in the 30 Doradus region of the Large Magellanic Cloud
DOI: 10.1051/0004-6361/201936361 Bibcode: 2020A&A...636A..54V

Kaper, L.; Sabbi, E.; de Mink, S. E. +13 more

The process of massive star (M ≥ 8 M) formation is still poorly understood. Observations of massive young stellar objects (MYSOs) are challenging due to their rarity, short formation timescale, large distances, and high circumstellar extinction. Here, we present the results of a spectroscopic analysis of a population of MYSOs in the La…

2020 Astronomy and Astrophysics
Gaia 10
Relations between Coronal Mass Ejections and the Photospheric Magnetic Field in Cycles 23 and 24
DOI: 10.3847/1538-4357/ab61fb Bibcode: 2020ApJ...889....1B

Bilenko, Irina A.

The number of coronal mass ejections (CMEs) and their parameters and cycle variations were investigated and compared to the photospheric magnetic field evolution in cycles 23 and 24. The Coordinated Data Analysis Workshops (CDAW) catalog of white-light CMEs detected by the Solar and Heliospheric Observatory/Large Angle and Spectrometric Coronagrap…

2020 The Astrophysical Journal
SOHO 10
Cold gas and dust: Hunting spiral-like structures in early-type galaxies
DOI: 10.1051/0004-6361/201935090 Bibcode: 2020A&A...636A...8Y

Duc, P. -A.; Peletier, R. F.; Serra, P. +1 more

Context. Observations of neutral hydrogen (H I) and molecular gas show that 50% of all nearby early-type galaxies contain some cold gas. Molecular gas is always found in small gas discs in the central region of the galaxy, while neutral hydrogen is often distributed in a low-column density disc or ring typically extending well beyond the stellar b…

2020 Astronomy and Astrophysics
Herschel 10
FEDReD. I. 3D extinction and stellar maps by Bayesian deconvolution
DOI: 10.1051/0004-6361/202037466 Bibcode: 2020A&A...641A..78B

Arenou, F.; Babusiaux, C.; Hottier, C. +2 more

Context. While Gaia enables us to probe the extended local neighbourhood in great detail, the thin disc structure at larger distances remains sparsely explored.
Aims: We aim here to build a non-parametric 3D model of the thin disc structures handling both the extinction and the stellar density simultaneously.
Methods: We developed a Baye…

2020 Astronomy and Astrophysics
Gaia 10
The absolute proper motions of the Arches and Quintuplet clusters
DOI: 10.1093/mnras/staa2327 Bibcode: 2020MNRAS.497.4733L

van der Marel, Roeland P.; Bellini, Andrea; Libralato, Mattia +2 more

Arches and Quintuplet are two young, massive clusters projected near the Galactic Centre. To date, studies focused on understanding their origin have been based on proper motions (PMs) derived in the clusters' reference frames and required some assumptions about their 3D motion. In this paper, we combine public PM catalogues of these clusters with…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 10
Characterizing X-Ray Properties of the Gamma-Ray Pulsar PSR J1418-6058 in the Rabbit Pulsar Wind Nebula
DOI: 10.3847/1538-4357/ab76c1 Bibcode: 2020ApJ...892....5K

An, Hongjun; Kim, Minjun

We report on X-ray studies of the gamma-ray pulsar PSR J1418-6058 in the Rabbit pulsar wind nebula (PWN) carried out using archival Chandra and XMM-Newton observations. A refined timing analysis performed with the 120 ks XMM-Newton data finds significant (p ≈ 10-7) pulsation at P ≈ 110 ms which is consistent with that measured with the …

2020 The Astrophysical Journal
XMM-Newton 10
A Method for the Estimation of f- and p-mode Parameters and Rotational Splitting Coefficients from Un-averaged Solar Oscillation Power Spectra
DOI: 10.3847/1538-4357/ab7a17 Bibcode: 2020ApJ...894...80R

Kosovichev, A. G.; Scherrer, P. H.; Larson, T. P. +3 more

We present a new methodology for the fitting of the peaks in solar oscillation power spectra that is equally well-suited for the estimation of low-, medium, and high-degree f- and p-mode parameters and frequency-splitting coefficients. The method can provide accurate input data over a wide portion of the dispersion plane for both structural and ro…

2020 The Astrophysical Journal
SOHO 10
AstroSat UVIT Detections of Chandra X-Ray Sources in M31
DOI: 10.3847/1538-4365/abadfb Bibcode: 2020ApJS..250...23L

Chen, Y.; Leahy, D. A.

An ultraviolet (UV) survey of M31 has been carried out during 2017-19 with the Ultra-Violet Imaging Telescope (UVIT) instrument on board the AstroSat Observatory. Here we match the M31 UVIT source catalog with the Chandra source catalog. We find 67 UVIT/Chandra sources detected in a varying number of UV and X-ray bands. The UV and X-ray photometry…

2020 The Astrophysical Journal Supplement Series
Gaia 10
Impact of a companion and of chromospheric emission on the shape of chromosome maps for globular clusters
DOI: 10.1051/0004-6361/201937212 Bibcode: 2020A&A...635A..52M

Martins, F.; Lardo, C.; Morin, J. +2 more

Context. Globular clusters (GCs) host multiple populations of stars that are well-separated in a photometric diagram - the chromosome map - built from specific Hubble Space Telescope (HST) filters. Stars from different populations feature at various locations on this diagram due to peculiar chemical compositions. Stars of the first population, wit…

2020 Astronomy and Astrophysics
eHST 10
Correlation of Structure and Stellar Properties of Galaxies in Stripe 82
DOI: 10.3847/1538-4357/aba82d Bibcode: 2020ApJ...899...89S

Ho, Luis C.; Sachdeva, Sonali; Shankar, Francesco +1 more

Establishing a correlation (or lack thereof) between the bimodal color distribution of galaxies and their structural parameters is crucial to understand the origin of bimodality. To achieve that, we have performed a 2D mass-based structural decomposition (bulge+disk) of all disk galaxies (total = 1263) in the Herschel imaging area of the Stripe 82…

2020 The Astrophysical Journal
Herschel 10