Search Publications

Searching for OB-type pre-supernova binary companions inside supernova remnants
DOI: 10.1093/mnras/stae1307 Bibcode: 2024MNRAS.531.4212D

Neuhäuser, R.; Mugrauer, M.; Ankay, A. +5 more

We searched for OB-runaway stars inside supernova remnants (SNRs) as a pre-supernova binary companion. As the majority of massive stars are found in close binary systems, a runaway star ejected by the orbital energy after the supernova (SN) is expected to be found. Considering a binary mass fraction, q = 0.25-1.0, the runaway star is likely to hav…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
The KALEIDOSCOPE survey: a new strong and weak gravitational lensing view of the massive galaxy cluster MACS J1423.8+2404
DOI: 10.1093/mnras/stae2069 Bibcode: 2024MNRAS.533.4500P

Mahler, Guillaume; Jauzac, Mathilde; Ebeling, Harald +6 more

We present a combined strong and weak gravitational-lensing analysis of the massive galaxy cluster MACS J1423.8+2404 ($z=0.545$, MACS J1423 hereafter), one of the most dynamically relaxed and massive cool-core clusters discovered in the MAssive Cluster Survey at

2024 Monthly Notices of the Royal Astronomical Society
eHST 1
Euclid view of the dusty star-forming galaxies at ≳ detected in wide area submillimetre surveys
DOI: 10.1093/mnras/stae976 Bibcode: 2024MNRAS.530.2292M

Cai, Zhen-Yi; Mitra, Dipanjan; Negrello, Mattia +1 more

We investigate the constraints provided by the Euclid space observatory on the physical properties of dusty star-forming galaxies (DSFGs) at $z\gtrsim 1.5$ detected in wide area submillimetre surveys with Herschel. We adopt a physical model for the high-z progenitors of spheroidal galaxies, which form the bulk of DSFGs at $z\gtrsim 1.5$. We improv…

2024 Monthly Notices of the Royal Astronomical Society
Herschel 1
A comprehensive study of orbital evolution of LMC X-4: existence of a second derivative of the orbital period
DOI: 10.1093/mnras/stae784 Bibcode: 2024MNRAS.529.4056J

Paul, Biswajit; Jain, Chetana; Sharma, Rahul

We report here results from pulse arrival time delay analysis of the eclipsing high-mass X-ray binary (HMXB) pulsar LMC X-4 using observations made with the Rossi X-ray Timing Explorer, XMM-Newton, NuSTAR (Nuclear Spectroscopic Telescope ARray), and AstroSat. Combining the orbital parameters determined from these observations with the historical m…

2024 Monthly Notices of the Royal Astronomical Society
INTEGRAL XMM-Newton 1
Cold electrons at a weakly outgassing comet
DOI: 10.1093/mnras/stae695 Bibcode: 2024MNRAS.529.2854S

Henri, P.; Galand, M.; Deca, J. +1 more

Throughout the Rosetta mission, cold electrons (<1 eV) were measured in the coma of comet 67P/Churyumov-Gerasimenko. Cometary electrons are produced at ~10 eV through photoionization or through electron-impact ionization collisions. The cold electron population is formed by cooling the warm population through inelastic electron-neutral collisio…

2024 Monthly Notices of the Royal Astronomical Society
Rosetta 1
Machine-learning applications for cataclysmic variable discovery in the ZTF alert stream
DOI: 10.1093/mnras/stad3768 Bibcode: 2024MNRAS.527.8633M

Copperwheat, C. M.; Darnley, M. J.; Mistry, D. +1 more

Cataclysmic variables (CV) encompass a diverse array of accreting white dwarf binary systems. Each class of CV represents a snapshot along an evolutionary journey, one with the potential to trigger a type Ia supernova event. The study of CVs offers valuable insights into binary evolution and accretion physics, with the rarest examples potentially …

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
The Gaia ultracool dwarf sample-IV. GTC/OSIRIS optical spectra of Gaia late-M and L dwarfs
DOI: 10.1093/mnras/stae2102 Bibcode: 2024MNRAS.534..695C

Caballero, J. A.; Montes, D.; Sarro, L. M. +20 more

As part of our comprehensive, ongoing characterization of the low-mass end of the main sequence in the Solar neighbourhood, we used the OSIRIS instrument at the 10.4 m Gran Telescopio Canarias to acquire low- and mid-resolution (R${\approx }$300 and R

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
Search for protostellar jets with UWISH2 in the molecular cloud complexes Vulpecula and IRDC G53.2
DOI: 10.1093/mnras/stae846 Bibcode: 2024MNRAS.530..515C

Tej, Anandmayee; Froebrich, Dirk; Samal, Manash +1 more

Jets and outflows are the early signposts of stellar birth. Using the UKIRT Wide Field Infrared Survey for H2 (UWISH2) at 2.12 µm, 127 outflows are identified in molecular cloud complexes Vulpecula OB1 and IRDC G53.2 covering 12 square degrees of the Galactic plane. Using multiwavelength data sets, from 1.2 to 70 µm, 79 youn…

2024 Monthly Notices of the Royal Astronomical Society
AKARI Herschel 1
The infalling elliptical galaxy M89: the chemical composition of the AGN disturbed hot atmosphere
DOI: 10.1093/mnras/stae065 Bibcode: 2024MNRAS.528.1500K

Werner, Norbert; Mernier, François; Ercan, E. Nihal +4 more

The chemical enrichment of X-ray-emitting hot atmospheres has hitherto been primarily studied in galaxy clusters. These studies revealed relative abundances of heavy elements that are remarkably similar to Solar. Here, we present measurements of the metal content of M89 (NGC 4552), an elliptical galaxy infalling into the Virgo cluster with a ~10 k…

2024 Monthly Notices of the Royal Astronomical Society
XMM-Newton 1
H2 molecular gas in the old planetary nebula NGC 3587
DOI: 10.1093/mnras/stad3841 Bibcode: 2024MNRAS.52710123R

Guerrero, M. A.; Toalá, J. A.; Ramos-Larios, G. +2 more

The acquisition of high-quality deep images of planetary nebulae (PNe) has allowed the detection of a wealth of small-scale features, which highlight the complexity of the formation history and physical processes shaping PNe. Here we present the discovery of three groups of clumps embedded within the nebular shell of the evolved PN NGC 3587, the O…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1