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JWST MIRI Imager Observations of Supernova SN 1987A
DOI: 10.3847/1538-4357/ad2770 Bibcode: 2024ApJ...965...51B

Fox, O. D.; Blommaert, J. A. D. L.; Larsson, J. +31 more

There exist very few mid-infrared (IR) observations of supernovae (SNe) in general. Therefore, SN 1987A, the closest visible SN in 400 yr, gives us the opportunity to explore the mid-IR properties of SNe, the dust in their ejecta, and the surrounding medium and to witness the birth of an SN remnant (SNR). The James Webb Space Telescope, with its h…

2024 The Astrophysical Journal
JWST 3
The influence of small bipolar magnetic regions on basic solar quantities
DOI: 10.1051/0004-6361/202245635 Bibcode: 2024A&A...683A..48H

Solanki, S. K.; Krivova, N. A.; Jiang, J. +2 more

Context. Understanding the evolution of the solar magnetic field is of great importance for heliosphere, dynamo, and irradiance studies, for example. While the contribution of the field in active regions (ARs) hosting sunspots to the Sun's large-scale field has been extensively modelled, we still lack a realistic model of the contribution of small…

2024 Astronomy and Astrophysics
SOHO 3
The Mass Dependence of Hα Emission and Stellar Spindown for Fully Convective M Dwarfs
DOI: 10.3847/1538-4357/ad3631 Bibcode: 2024ApJ...966..231P

Latham, David W.; Berlind, Perry; Calkins, Michael L. +4 more

Fully convective M dwarfs typically remain rapidly rotating and magnetically active for billions of years, followed by an abrupt and mass-dependent transition to slow rotation and quiescence. A robust understanding of this process is complicated by difficulties in estimating M dwarf ages and potential dependencies on other variables such as birth …

2024 The Astrophysical Journal
Gaia 3
The Orbit of NGC 5907 ULX-1
DOI: 10.3847/1538-4357/ad320a Bibcode: 2024ApJ...965...78B

Wolter, Anna; Pintore, Fabio; Mereghetti, Sandro +13 more

We report on the orbit of the binary system powering the most extreme ultraluminous X-ray pulsar known to date: NGC 5907 ULX-1 (hereafter ULX1). ULX1 has been the target of a substantial multi-instrument campaign, mainly in the X-ray band, but no clear counterparts are known in other bands. Although ULX1 is highly variable and pulsations can be tr…

2024 The Astrophysical Journal
XMM-Newton 3
A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3
DOI: 10.1093/mnras/stae1155 Bibcode: 2024MNRAS.530.4578B

Berta, S.; Ivison, R. J.; Omont, A. +38 more

We report on deep SCUBA-2 observations at 850 $\mu$m and NOrthern Extended Millimetre Array (NOEMA) spectroscopic measurements at 2 mm of the environment surrounding the luminous, massive (M* ≈ 2 × 1011 M) Herschel-selected source HerBS-70. This source was revealed by previous NOEMA observations to be a binary sys…

2024 Monthly Notices of the Royal Astronomical Society
Herschel 3
The "Magnificent Seven" X-Ray Isolated Neutron Stars Revisited. I. Improved Timing Solutions and Pulse Profile Analysis
DOI: 10.3847/1538-4357/ad452b Bibcode: 2024ApJ...969...53B

Bogdanov, Slavko; Ho, Wynn C. G.

We present the first systematic X-ray pulse timing analysis of the six members of the so-called "Magnificent Seven" nearby thermally emitting isolated neutron stars (XINS) with detected pulsations. Using the extensive collection of archival XMM-Newton, Chandra, and NICER observations spanning over two decades, we obtain the first firm measurement …

2024 The Astrophysical Journal
XMM-Newton 3
Search for Classical Cepheids in Galactic Open Clusters and Calibration of the Period–Wesenheit–Metallicity Relation in the Gaia Bands
DOI: 10.3847/1538-3881/ad50d3 Bibcode: 2024AJ....168...34W

Xu, Ye; Liu, Dejian; Hao, Chaojie +3 more

It is beneficial to calibrate the period–Wesenheit–metallicity relation (PWZR) of Delta Cephei stars (DCEPs), i.e., classical Cepheids, using accurate parallaxes of associated open clusters (OCs) from Gaia data release 3 (DR3). To this aim, we obtain a total of 43 OC–DCEPs (including 33 fundamental mode, 9 first overtone mode, and 1 multimode DCEP…

2024 The Astronomical Journal
Gaia 3
Detailed cool star flare morphology with CHEOPS and TESS***
DOI: 10.1051/0004-6361/202348951 Bibcode: 2024A&A...686A.239B

Alonso, R.; Deleuil, M.; Erikson, A. +79 more

Context. White-light stellar flares are proxies for some of the most energetic types of flares, but their triggering mechanism is still poorly understood. As they are associated with strong X and ultraviolet emission, their study is particularly relevant to estimate the amount of high-energy irradiation onto the atmospheres of exoplanets, especial…

2024 Astronomy and Astrophysics
CHEOPS Gaia 3
Revisit of 77 Clusters Candidates with Multiple Main Sequences using Gaia DR3
DOI: 10.3847/1538-3881/acf99f Bibcode: 2024AJ....167...44C

Li, Zhongmu; Chen, Jing; Zhang, Su +2 more

Gaia DR3 data provide the latest and full astrometric data for more than 1.5 billion sources, and these allow us to revisit the 77 special open cluster candidates collected from LISC star cluster catalog. According to their unclear color-magnitude-diagram (CMD) morphology, they are difficult to be ensured as real open clusters (OCs), and their clu…

2024 The Astronomical Journal
Gaia 3
JWST observations of the Horsehead photon-dominated region. I. First results from multi-band near- and mid-infrared imaging
DOI: 10.1051/0004-6361/202449198 Bibcode: 2024A&A...687A...4A

Abergel, A.; Bouchet, P.; Brandl, B. R. +14 more

Context. The James Webb Space Telescope (JWST) has captured the sharpest infrared images ever taken of the Horsehead nebula, a prototypical moderately irradiated photon-dominated region (PDR) that is fully representative of most of the UV-illuminated molecular gas in the Milky Way and star-forming galaxies.
Aims: We investigate the impact of …

2024 Astronomy and Astrophysics
Gaia eHST JWST 3