Search Publications

Discovery and timing of pulsar J2016+3711 in supernova remnant CTB 87 with FAST
DOI: 10.1093/mnras/stae351 Bibcode: 2024MNRAS.528.6761L

Li, Di; Zhou, Ping; Chen, Yang +4 more

We report on our discovery of the radio pulsar, PSR J2016+3711, in supernova remnant (SNR) CTB 87, with a ~10.8σ significance of pulses, which confirms the compact nature of the X-ray point source in CTB 87. It is the first pulsar discovered in SNRs using Five-hundred-meter Aperture Spherical radio Telescope (FAST). Its integrated radio pulse prof…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
Asteroid reflectance spectra from Gaia DR3: Near-UV in primitive asteroids
DOI: 10.1051/0004-6361/202348752 Bibcode: 2024A&A...686A..76T

Tatsumi, E.; Tanga, P.; Licandro, J. +4 more

Context. In the context of charge-coupled devices (CCDs), the ultraviolet (UV) region has mostly remained unexplored after the 1990s. Gaia DR3 offers the community a unique opportunity to explore tens of thousands of asteroids in the near-UV as a proxy of the UV absorption. This absorption has been proposed in previous works as a diagnostic of hyd…

2024 Astronomy and Astrophysics
Gaia 4
Ground- and Space-based Dust Observations of VV 191 Overlapping Galaxy Pair
DOI: 10.3847/1538-3881/ad39c4 Bibcode: 2024AJ....167..263R

Grogin, Norman A.; Holwerda, Benne W.; Koekemoer, Anton M. +12 more

The Balmer decrement (Hα/Hβ) provides a constraint on attenuation, the cumulative effects of dust grains in the ISM. The ratio is a reliable spectroscopic tool for deriving the dust properties of galaxies that determine many different quantities such as star formation rate, metallicity, and SED models. Here, we measure independently both the atten…

2024 The Astronomical Journal
eHST JWST 4
The Kraft Break Sharply Divides Low-mass and Intermediate-mass Stars
DOI: 10.3847/1538-4357/ad6b0d Bibcode: 2024ApJ...973...28B

White, Russel J.; Beyer, Alexa C.

Main-sequence stars transition at mid-F spectral types from slowly rotating (cooler stars) to rapidly rotating (hotter stars), a transition known as the Kraft Break and attributed to the disappearance of the outer convective envelope, causing magnetic braking to become ineffective. To define this Break more precisely, we assembled spectroscopic me…

2024 The Astrophysical Journal
Gaia 4
Catalogue of BRITE-Constellation targets. I. Fields 1 to 14 (November 2013-April 2016)
DOI: 10.1051/0004-6361/202348236 Bibcode: 2024A&A...683A..49Z

Smolec, R.; Handler, G.; Wade, G. A. +25 more

Context. The BRIght Target Explorer (BRITE) mission collects photometric time series in two passbands with the aim of investigating stellar structure and evolution. Since their launches in the years 2013 and 2014, the constellation of five BRITE nano-satellites has observed a total of more than 700 individual bright stars in 64 fields. Some target…

2024 Astronomy and Astrophysics
Gaia 4
A Close Look at Lyα Emitters with JWST/NIRCam at z ≈ 3.1
DOI: 10.3847/1538-4357/ad3822 Bibcode: 2024ApJ...966..210L

Jiang, Linhua; Wuyts, Stijn; Huang, Jia-Sheng +2 more

We study 10 spectroscopically confirmed Lyα emitters (LAEs) at z ≈ 3.1 in the Ultra Deep Survey field, covered by the James Webb Space Telescope/NIRCam in the Public Release Imaging for Extragalactic Research program. All LAEs are detected in all NIRCam bands from F090W to F444W, corresponding to rest frame wavelengths of 2200 Å to 1.2 µm. B…

2024 The Astrophysical Journal
eHST JWST 4
Radial velocities from Gaia BP/RP spectra
DOI: 10.1051/0004-6361/202348406 Bibcode: 2024A&A...684A..29V

Kuijken, Konrad; Koposov, Sergey E.; Verberne, Sill +3 more


Aims: The Gaia mission has provided us full astrometric solutions for over 1.5B sources. However, only the brightest 34M of them have radial velocity measurements. This paper aims to close that gap by obtaining radial velocity estimates from the low-resolution BP/RP spectra that Gaia now provides. These spectra are currently published for abo…

2024 Astronomy and Astrophysics
Gaia 4
Discovery of a Second Eclipsing, ​​​​​Bursting Neutron Star Low-mass X-Ray Binary in the Globular Cluster Terzan 6
DOI: 10.3847/1538-4357/ad2f3d Bibcode: 2024ApJ...966..217V

Bahramian, Arash; Homan, Jeroen; Heinke, Craig O. +4 more

We have analyzed Chandra and Suzaku observations of the globular cluster Terzan 6, made when the recurrent transient GRS 1747–312 was in quiescence. Our analysis reveals the presence of a second eclipsing, bursting neutron star low-mass X-ray binary in the central regions of the cluster, in addition to GRS 1747–312. The new source, which we name T…

2024 The Astrophysical Journal
Gaia Suzaku eHST 4
Double red giant branch and red clump features of Galactic disc stellar populations with Gaia GSP-Spec
DOI: 10.1051/0004-6361/202449443 Bibcode: 2024A&A...692A.235R

Recio-Blanco, A.; de Laverny, P.; Palicio, P. A. +4 more

Context. The bimodality of the Milky Way disc, in the form of a thick short disc and a thinner more radially extended one, encrypts the complex internal evolution of our Galaxy and its interaction with the environment. Aims. To disentangle the different competing physical processes at play in Galactic evolution, a detailed chrono-chemical-kinemati…

2024 Astronomy and Astrophysics
Gaia 4
The Interplay Between Collisionless Magnetic Reconnection and Turbulence
DOI: 10.1007/s11214-024-01124-8 Bibcode: 2024SSRv..220...90S

Hasegawa, H.; Khotyaintsev, Yu. V.; Graham, D. B. +13 more

Alongside magnetic reconnection, turbulence is another fundamental nonlinear plasma phenomenon that plays a key role in energy transport and conversion in space and astrophysical plasmas. From a numerical, theoretical, and observational point of view there is a long history of exploring the interplay between these two phenomena in space plasma env…

2024 Space Science Reviews
Cluster 4