Results 61 to 70 of about 12,394 (217)
Abstract A new 80‐site magnetotelluric (MT) survey, integrated with reprocessed seismic reflection profiles, across the supergiant Timmins‐Porcupine gold camp of the Abitibi greenstone belt (AGB) was conducted to investigate the architecture of crustal‐scale structures.
A. Q. Adetunji +6 more
wiley +1 more source
Abstract The discovery of new economic copper deposits is critical for the development of renewable energy infrastructure and zero‐emissions transport. The majority of existing copper mines are located within current or extinct continental arc systems, but our understanding of the tectonic and geodynamic conditions favoring the formation of porphyry ...
Ehsan Farahbakhsh +6 more
wiley +1 more source
XMM‐Newton Observations of the Peculiar Be X‐Ray Binary A0538‐66
ABSTRACT A0538‐66 is a neutron star/Be x‐ray binary located in the Large Magellanic Cloud and, since its discovery in the 70s, it showed a peculiar behavior that makes it a unique object in the high‐mass x‐ray binaries scene: the extremely eccentric orbit (e=0.72$$ e=0.72 $$), the short spin period of the neutron star (P=69$$ P=69 $$ ms), the episodes ...
Michela Rigoselli +3 more
wiley +1 more source
Beyond Accretion Limits: The Rise of Pulsating Gems
ABSTRACT The discovery of several ultraluminous X‐ray sources exhibiting fast and rapidly evolving X‐ray pulsations unequivocally associates these sources with accreting neutron stars orbiting relatively massive companion stars (> 8M ⊙$$ {}_{\odot } $$).
Gian Luca Israel +26 more
wiley +1 more source
The MACHO Project 9 Million Star Color-Magnitude Diagram of the Large Magellanic Cloud [PDF]
We present a 9 million star color-magnitude diagram (9M CMD) of the LMC bar. The 9M CMD reveals a complex superposition of different age and metallicity stellar populations, with important stellar evolutionary phases occurring over 3 orders of magnitude ...
A. B. Tomaney +58 more
core +2 more sources
The yellow hypergiants are found in a stage between the massive Red Supergiants and the Wolf-Rayet stars. This review addresses current issues concerning the evolution of massive stars, concentrating on the transitional post-Red Supergiant phase.
Oudmaijer, Rene +3 more
openaire +2 more sources
Weakly Magnetized Accreting Neutron Stars as Seen by IXPE
ABSTRACT The Imaging X‐ray Polarimetry Explorer, recently awarded by the American Astronomical Society with the Bruno Rossi prize, observed several accreting neutron stars in X‐ray binaries during the first 2 years of its prime mission. Results obtained for weakly magnetized neutron stars allow us to model the geometry and the physical status of the ...
Alessandro Di Marco +1 more
wiley +1 more source
Modeling the near-infrared lines of O-type stars [PDF]
We use a grid of 30 line-blanketed unified stellar photosphere and wind models for O-type stars; computed with the code CMFGEN in order to evaluate its potential in the near-infrared spectral domain. The grid includes dwarfs, giants and supergiants.
de Koter, A. +3 more
core +2 more sources
Stellar winds in a-type supergiants [PDF]
The contribution of A supergiant stars to the return of mass and energy to the interstellar medium is not very important. Abbott (1982) analised a sample of early stars and concluded that B and A supergiants provided less than 8 % of the mass input to the ISM by stellar winds.
A. Talavera, A.I. Gomez de Castro
openaire +1 more source
Insulin‐like growth Factor 1 (IGF1) plays a vital role in vertebrate growth, and its sexually biased expression may influence the development and evolution of sexual size dimorphism (SSD). To investigate the role of IGF1 in regulating the growth of the Chinese soft‐shelled turtle (Pelodiscus sinensis), this study quantified IGF1 mRNA abundance across ...
Dan Zeng +7 more
wiley +1 more source

