A spectroscopic survey of Herbig Ae/Be stars with X-shooter - I. Stellar parameters and accretion rates [PDF]
JRF gratefully acknowledges a studentship from the Science and Technology Facilities Council of the UK. JDI gratefully acknowledges funding from the European Union FP7-2011 under grant agreement no.
van den Ancker, M. E. +9 more
core +1 more source
Topics in Core-Collapse Supernova Theory: The Formation of Black Holes and the Transport of Neutrinos [PDF]
Core-Collapse Supernovae are one of the most complex astrophysical systems in the universe. They deeply entwine aspects of physics and astrophysics that are rarely side by side in nature.
O'Connor, Evan Patrick
core +1 more source
The Nature of Blue Stars with Mid-infrared Excesses in the Large Magellanic Cloud
We present low-resolution optical spectra and classifications of 92 blue objects with mid-infrared excesses in the Large Magellanic Cloud. The majority of these objects were selected with the criteria of U − B < 0 and V < 17 from the potential young ...
Ryoko Ishioka +5 more
doaj +1 more source
A near-infrared interferometric survey of debris disc stars. III. First statistics based on 42 stars observed with CHARA/FLUOR [PDF]
peer reviewedContext. Dust is expected to be ubiquitous in extrasolar planetary systems due to the dynamical activity of minor bodies. Inner dust populations are, however, still poorly known due to the high contrast and small angular separation with ...
Mérand, Antoine +63 more
core +1 more source
Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars
In 2013 a dearth of close-in planets around fast-rotating host stars was found using statistical tests on Kepler data. The addition of more Kepler and Transiting Exoplanet Survey Satellite (TESS) systems in 2022 filled this region of the diagram of stellar rotation period ( P rot ) versus the planet orbital period ( P orb ).
García, R. +10 more
openaire +4 more sources
Evidence for Misalignment between Debris Disks and Their Host Stars
We place lower limits on the obliquities between debris disks and their host stars for 31 systems by comparing their disk and stellar inclinations.
Spencer A. Hurt, Meredith A. MacGregor
doaj +1 more source
Quantitative Stellar Spectral Classification. II. Early Type Stars
The method developed by Stock and Stock (1999) for stars of spectral types A to K to derive absolute magnitudes and intrinsic colors from the equivalent widths of absorption lines in stellar spectra is extended to B-type stars. Spectra of this type of stars for which the Hipparcos Catalogue gives parallaxes with an error of less than 20% were observed ...
Stock, M. J. +3 more
openaire +2 more sources
NOT has been an important telescope in studying galactic nebulae and stellar outflows since its inauguration more than 30 years ago. Superb observational capabilities provide simultaneous imaging and 2D spectral data, which is indispensable when ...
Djupvik, Amanda +6 more
core +1 more source
A Census of the Stellar Populations in the Sco-Cen Complex
I have used high-precision photometry and astrometry from the early installment of the third data release of Gaia (EDR3) to perform a survey for members of the stellar populations within the Sco-Cen complex, which consist of Upper Sco, UCL/LCC, the V1062
K. L. Luhman
doaj +1 more source
Stellar parameters of early-M dwarfs from ratios of spectral features at optical wavelengths [PDF]
This work was supported by the Italian Ministry of Education, University, and Research through the Premiale HARPS-N research project under grant Ricerca di pianeti intorno a stelle di piccola massa. M.P. and I.R.
Southworth, J. +31 more
core +1 more source

