Search Publications

Shiva and Shakti: Presumed Proto-Galactic Fragments in the Inner Milky Way
DOI: 10.3847/1538-4357/ad1885 Bibcode: 2024ApJ...964..104M

Rix, Hans-Walter; Malhan, Khyati

Using Gaia Data Release 3 astrometry and spectroscopy, we study two new substructures in the orbit–metallicity space of the inner Milky Way: Shakti and Shiva. They were identified as two confined, high-contrast overdensities in the (L z , E) distribution of bright (G < 16) and metal-poor (‑2.5 < [M/H] < ‑ 1.0) stars. Both have…

2024 The Astrophysical Journal
Gaia 22
On the Mesoscale Structure of Coronal Mass Ejections at Mercury's Orbit: BepiColombo and Parker Solar Probe Observations
DOI: 10.3847/1538-4357/ad1ab4 Bibcode: 2024ApJ...963..108P

Dresing, Nina; Nieves-Chinchilla, Teresa; Weiss, Andreas J. +27 more

On 2022 February 15, an impressive filament eruption was observed off the solar eastern limb from three remote-sensing viewpoints, namely, Earth, STEREO-A, and Solar Orbiter. In addition to representing the most-distant observed filament at extreme ultraviolet wavelengths—captured by Solar Orbiter's field of view extending to above 6 R

2024 The Astrophysical Journal
BepiColombo SOHO SolarOrbiter 22
Binary stars in the new millennium
DOI: 10.1016/j.ppnp.2023.104083 Bibcode: 2024PrPNP.13404083C

Han, Zhanwen; Chen, Xuefei; Liu, Zhengwei

Binary stars are as common as single stars. Binary stars are of immense importance to astrophysicists because that they allow us to determine the masses of the stars independent of their distances. They are the cornerstone of the understanding of stellar evolutionary theory and play an essential role in cosmic distance measurement, galactic evolut…

2024 Progress in Particle and Nuclear Physics
Gaia 22
MIDIS: The Relation between Strong (Hβ + [O III]) Emission, Star Formation, and Burstiness around the Epoch of Reionization
DOI: 10.3847/1538-4357/ad4eb2 Bibcode: 2024ApJ...969..159C

Nørgaard-Nielsen, H. U.; Östlin, G.; Güdel, M. +25 more

We investigate the properties of strong (Hβ + [O III]) emitters before and after the end of the "Epoch of Reionization" from z = 8 to z = 5.5. We make use of ultradeep JWST/NIRCam imaging in the parallel field (P2) of the MIRI Deep Imaging Survey (MIDIS) in the Hubble eXtreme Deep Field (H-XDF), in order to select prominent (Hβ + [O III]) emitters…

2024 The Astrophysical Journal
eHST JWST 22
Lyman continuum leaker candidates at z ∼ 3-4 in the HDUV based on a spectroscopic sample of MUSE LAEs
DOI: 10.1051/0004-6361/202346656 Bibcode: 2024A&A...684A..42K

Oesch, P. A.; Illingworth, G. D.; Verhamme, A. +15 more

Context. In recent years, a number of Lyman continuum (LyC) leaker candidates have been found at intermediate redshifts, providing insight into how the Universe was reionised at early cosmic times. There are now around 100 known LyC leakers at all redshifts, which enables us to analyse their properties statistically.
Aims: Here, we identify n…

2024 Astronomy and Astrophysics
eHST 22
JWST MIRI Detections of Hα and [O III] and a Direct Metallicity Measurement of the z = 10.17 Lensed Galaxy MACS0647‑JD
DOI: 10.3847/1538-4357/ad6562 Bibcode: 2024ApJ...973...81H

Costantin, Luca; Hutchison, Taylor A.; Larson, Rebecca L. +30 more

JWST spectroscopy has revolutionized our understanding of galaxies in the early Universe. Covering wavelengths up to 5.3 µm, NIRSpec can detect rest-frame optical Hα emission lines out to z = 7 and [O III] to z = 9.5. Observing these lines in more distant galaxies requires longer wavelength spectroscopy with MIRI. Here we present MIRI Medium…

2024 The Astrophysical Journal
eHST JWST 22
Probing orbits of stellar mass objects deep in galactic nuclei with quasiperiodic eruptions. II. Population analysis
DOI: 10.1103/PhysRevD.110.083019 Bibcode: 2024PhRvD.110h3019Z

Pan, Zhen; Zhou, Cong; Huang, Lei +2 more

Quasiperiodic eruptions (QPEs) are intense repeating soft x-ray bursts with recurrence times about a few hours to a few weeks from galactic nuclei. Though the debates on the origin of QPEs have not completely settled down, more and more analyses favor the interpretation that QPEs are the result of collisions between a stellar mass object (a stella…

2024 Physical Review D
XMM-Newton 22
Abundant hydrocarbons in the disk around a very-low-mass star
DOI: 10.1126/science.adi8147 Bibcode: 2024Sci...384.1086A

Waters, L. B. F. M.; Olofsson, G.; Kamp, I. +40 more

Very-low-mass stars (those less than 0.3 solar masses) host orbiting terrestrial planets more frequently than other types of stars. The compositions of those planets are largely unknown but are expected to relate to the protoplanetary disk in which they form. We used James Webb Space Telescope mid-infrared spectroscopy to investigate the chemical …

2024 Science
XMM-Newton JWST 22
Emission lines due to ionizing radiation from a compact object in the remnant of Supernova 1987A
DOI: 10.1126/science.adj5796 Bibcode: 2024Sci...383..898F

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

The nearby Supernova 1987A was accompanied by a burst of neutrino emission, which indicates that a compact object (a neutron star or black hole) was formed in the explosion. There has been no direct observation of this compact object. In this work, we observe the supernova remnant with JWST spectroscopy, finding narrow infrared emission lines of a…

2024 Science
Gaia JWST 22
The Star-forming Main Sequence in JADES and CEERS at z > 1.4: Investigating the Burstiness of Star Formation
DOI: 10.3847/1538-4357/ad8ba4 Bibcode: 2024ApJ...977..133C

Shapley, Alice E.; Reddy, Naveen A.; Sanders, Ryan L. +5 more

We have used public JWST/NIRSpec and JWST/NIRCam observations from the CEERS and JADES surveys in order to analyze the star-forming main sequence (SFMS) over the redshift range 1.4 ≤ z < 7. We calculate the star formation rates (SFRs) of the galaxy sample using three approaches: Balmer line luminosity, spectral energy distribution (SED) fitting…

2024 The Astrophysical Journal
eHST JWST 22