Search Publications

Understanding the star formation efficiency in dense gas: Initial results from the CAFFEINE survey with ArTéMiS
DOI: 10.1051/0004-6361/202449908 Bibcode: 2024A&A...688A.163M

Roussel, H.; André, Ph.; Arzoumanian, D. +9 more

Context. Despite recent progress, the question of what regulates the star formation efficiency (SFE) in galaxies remains one of the most debated problems in astrophysics. According to the dominant picture, star formation (SF) is regulated by turbulence and feedback, and the SFE is ~1-2% or less per local free-fall time on all scales from Galactic …

2024 Astronomy and Astrophysics
Herschel 7
Small-scale magnetic flux emergence preceding a chain of energetic solar atmospheric events
DOI: 10.1051/0004-6361/202348894 Bibcode: 2024A&A...686A.218N

Rouppe van der Voort, L. H. M.; Joshi, R.; Froment, C. +4 more

Context. Advancements in instrumentation have revealed a multitude of small-scale extreme-ultraviolet (EUV) events in the solar atmosphere and considerable effort is currently undergoing to unravel them.
Aims: Our aim is to employ high-resolution and high-sensitivity magnetograms to gain a detailed understanding of the magnetic origin of such…

2024 Astronomy and Astrophysics
Hinode IRIS SolarOrbiter 7
Radio Jet Feedback on the Inner Disk of Virgo Spiral Galaxy Messier 58
DOI: 10.3847/1538-4357/ad1242 Bibcode: 2024ApJ...962..196O

Togi, Aditya; Rich, R. Michael; Román, Javier +9 more

Spitzer spectral maps reveal a disk of highly luminous, warm (>150 K) H2 in the center of the massive spiral galaxy Messier 58, which hosts a radio-loud active galactic nucleus (AGN). The inner 2.6 kpc of the galaxy appears to be overrun by shocks from the radio jet cocoon. Gemini NIRI imaging of the H2 1–0 S(1) emission l…

2024 The Astrophysical Journal
eHST 7
NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at 1.5 < z < 4 in the COSMOS field
DOI: 10.1051/0004-6361/202450760 Bibcode: 2024A&A...690A..55S

Daddi, Emanuele; Schinnerer, Eva; Cai, Zheng +41 more

The NOrthern Extended Millimeter Array (NOEMA) formIng Cluster survEy (NICE) is a NOEMA large programme targeting 69 massive galaxy group candidates at z > 2 over six deep fields with a total area of 46 deg2. Here we report the spectroscopic confirmation of eight massive galaxy groups at redshifts 1.65 ≤ z ≤ 3.61 in the Cosmic Evolut…

2024 Astronomy and Astrophysics
Herschel 7
SED Analysis of the Old Open Cluster NGC 188
DOI: 10.26650/PAR.2024.00002 Bibcode: 2024PARep...2....1C

Çınar, Deniz Cennet; Tasdemir, Seval; Koc, Seliz +1 more

In this study, we investigate the fundamental astrophysical parameters of the old open cluster NGC 188 using two complementary methods: isochron fitting and spectral energy distribution (SED) analysis. Using photometric, astrometric, and spectroscopic data from the {\it Gaia} Data Release 3 \citep[DR3,][]{Gaia_DR3}, we identified 868 most likely m…

2024 Physics and Astronomy Reports
Gaia 7
The first measurements of carbon isotopic ratios in post-RGB stars: SZ Mon and DF Cyg
DOI: 10.1093/mnras/stae791 Bibcode: 2024MNRAS.530..761M

Ventura, Paolo; Masseron, Thomas; Van Winckel, Hans +4 more

Dusty post-red giant branch (post-RGB) stars are low- and intermediate-mass stars where the RGB evolution was prematurely terminated by a poorly understood binary interaction. These binary stars are considered to be low-luminosity analogues of post-asymptotic giant branch (post-AGB) binary stars. In this study, we investigated the chemical composi…

2024 Monthly Notices of the Royal Astronomical Society
AKARI Gaia 7
Coronal Holes, Footpoint Reconnection, and the Origin of the Slow (and Fast) Solar Wind
DOI: 10.1007/s11207-024-02300-3 Bibcode: 2024SoPh..299...54W

Wang, Y. -M.

The tendency for low-speed solar wind to show greater spatiotemporal variability and different compositional properties from high-speed wind has led to the prevailing idea of a bimodal solar wind, in which fast wind comes from coronal holes and slow wind comes from coronal streamers. We present observational evidence that most of the slow wind ori…

2024 Solar Physics
SolarOrbiter 7
Galaxies decomposition with spiral arms - II. A multiwavelength case study of M 51
DOI: 10.1093/mnras/stae108 Bibcode: 2024MNRAS.528.1276M

Gontcharov, George A.; Mosenkov, Aleksandr V.; Savchenko, Sergey S. +7 more

Spiral structure can contribute significantly to a galaxy's luminosity. However, only rarely are proper photometric models of spiral arms used in decompositions. As we show in the previous work, including the spirals as a separate component in a photometric model of a galaxy would both allow to obtain their structural parameters, and reduce the sy…

2024 Monthly Notices of the Royal Astronomical Society
Herschel 7
A catalogue of Galactic GEMS: Globular cluster Extra-tidal Mock Stars
DOI: 10.1093/mnras/stae203 Bibcode: 2024MNRAS.528.5189G

Speagle, Joshua S.; Lane, James M. M.; Webb, Jeremy J. +2 more

This work presents the Globular cluster Extra-tidal Mock Star (GEMS) catalogue of extra-tidal stars and binaries created via three-body dynamical encounters in globular cluster cores. Using the particle-spray code Corespray, we sample $N=50\, 000$ extra-tidal stars and escaped recoil binaries for 159 Galactic globular clusters. Sky positions, kine…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 7
Discovery and follow-up of ASASSN-23bd (AT 2023clx): the lowest redshift and luminosity optically selected tidal disruption event
DOI: 10.1093/mnras/stae1121 Bibcode: 2024MNRAS.530.4501H

Kochanek, C. S.; Galbany, L.; Brown, P. J. +23 more

We report the All-Sky Automated Survey for SuperNovae discovery of the tidal disruption event (TDE) ASASSN-23bd (AT 2023clx) in NGC 3799, a LINER galaxy with no evidence of strong active galactic nucleus (AGN) activity over the past decade. With a redshift of z = 0.01107 and a peak ultraviolet (UV)/optical luminosity of (5.4 ± 0.4) × 1042

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 7