Search results for "circumstellar mater"

showing 2 items of 2 documents

DISTRIBUTION OF CARBON STARS IN THE GALAXY

2018

A search for new faint carbon (C) stars in the Polar region δ > 55o has been accomplished by obtaining objective prism spectra in the near infrared 550 -- 900 nm on images of CCD camera of Baldone Schmidt telescope of Astrophysical observatory. The positions of stars   having color indices (J – K) > 1.3 mag in Two Micron All Sky Infrared Survey (2MASS) were selected to pick out suspicious carbon stars.Our survey is limited in brightness by J < 10 mag. 24 new carbon stars were found and their characteristics obtained. The correlative relation between Teff  and spectral gradient [757 – 685] was confirmed. Such characteristics as Teff, distance from the Sun, absolute Mk  were obtained…

Absolute magnitudePhysicsBrightnessInfraredcircumstellar materlcsh:Astronomymedia_common.quotation_subjectnear infraredAstrophysics::Instrumentation and Methods for Astrophysicsabsolute magnitudeAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSchmidt cameraCarbon starGalaxylcsh:QB1-991StarsSkyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsdistanceAstrophysics::Galaxy Astrophysicscarbon starsmedia_commoncircumstellar mater; near infrared; carbon stars; absolute magnitude; distanceOdessa Astronomical Publications
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Photometric and Spectroscopic Properties of Type Ia Supernova 2018oh with Early Excess Emission from the $Kepler$ 2 Observations

2019

Supernova (SN) 2018oh (ASASSN-18bt) is the first spectroscopically-confirmed type Ia supernova (SN Ia) observed in the $Kepler$ field. The $Kepler$ data revealed an excess emission in its early light curve, allowing to place interesting constraints on its progenitor system (Dimitriadis et al. 2018, Shappee et al. 2018b). Here, we present extensive optical, ultraviolet, and near-infrared photometry, as well as dense sampling of optical spectra, for this object. SN 2018oh is relatively normal in its photometric evolution, with a rise time of 18.3$\pm$0.3 days and $\Delta$m$_{15}(B)=0.96\pm$0.03 mag, but it seems to have bluer $B - V$ colors. We construct the "uvoir" bolometric light curve hav…

DATA RELEASEULTRAVIOLETFACTORY OBSERVATIONSFOS: Physical sciencesAstrophysicsType (model theory)medicine.disease_causeSN 2011FE01 natural sciencesLuminosityPhotometry (optics)individual (SN 2018oh) [supernovae]supernovae: generalCIRCUMSTELLAR MATERIAL0103 physical sciencesmedicineSPECTRAAbsorption (logic)Ejecta010303 astronomy & astrophysicssupernovae: individualQCSolar and Stellar Astrophysics (astro-ph.SR)QBLIGHT CURVESHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHIGH-VELOCITY FEATURES010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveSupernovaAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceIMPROVED DISTANCESWHITE-DWARF MODELSAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]general [supernovae]Ultraviolet
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