Results 111 to 120 of about 7,751,768 (367)
Modeling the TESS Light Curve of Ap Si Star MX TrA
The TESS light curve of the silicon Ap star MX TrA was modeled using the observational surface distribution of silicon, iron, helium, and chromium obtained previously with the Doppler Imaging technique.
Yury Pakhomov+3 more
doaj +1 more source
SYNTHETIC LIGHT CURVE OF R CORONAE BOREALIS
The model for brightness variations of CrB is proposed.
A. F. Pugach, G. U. Kovalchuk
doaj +1 more source
WASP light curve of the eclipsing binary VZ CVn [PDF]
The WASP light curve of the eclipsing binary VZ CVn, consisting of more than 14000 individual observations, is analyzed for photometric elements using the modeling code of Đurašević (1992).
Latković O.
doaj +1 more source
Can Kilonova Light Curves Be Standardized? [PDF]
Abstract Binary neutron star (NS) mergers have been recently confirmed to be the progenitors of the optical transients kilonovae (KNe). KNe are powered by the radioactive decay of neutron-rich elements (r-process elements), which are believed to be the product of disruption of NSs during their merger.
Rahul Kashyap+3 more
openaire +3 more sources
VALIDATION OF KEPLER'S MULTIPLE PLANET CANDIDATES. III. LIGHT CURVE ANALYSIS AND ANNOUNCEMENT OF HUNDREDS OF NEW MULTI-PLANET SYSTEMS [PDF]
The Kepler mission has discovered more than 2500 exoplanet candidates in the first two years of spacecraft data, with approximately 40% of those in candidate multi-planet systems.
J. Rowe+35 more
semanticscholar +1 more source
This study reveals how prime editing guide RNA (pegRNA) secondary structure and reverse transcriptase template length affect prime editing efficiency in correcting the phospholamban R14del cardiomyopathy‐associated mutation. Insights support the design of structurally optimized enhanced pegRNAs for precise gene therapy.
Bing Yao+7 more
wiley +1 more source
IntroductionThe first multi-color photometric observations and low-resolution spectra of the Algol-type short-period eclipsing binary systems IWUMa and V367 Gem are presented here.
Xiao-Man Tian+3 more
doaj +1 more source
Polarization and light curve variability: the "patchy shell" model
Recent advances in early detection and detailed monitoring of GRB afterglows have revealed variability in some afterglow light curves. One of the leading models for this behavior is the patchy shell model.
Ehud Nakar+3 more
core +1 more source
On the Light Curves of AM CVn [PDF]
Submitted to "Acta Astronomica"
openaire +3 more sources
SUPERNOVAE WITH TWO PEAKS IN THE OPTICAL LIGHT CURVE AND THE SIGNATURE OF PROGENITORS WITH LOW-MASS EXTENDED ENVELOPES [PDF]
Early observations of supernova light curves are powerful tools for shedding light on the pre-explosion structures of their progenitors and their mass-loss histories just prior to explosion.
E. Nakar, A. Piro
semanticscholar +1 more source