Výsledky vyhledávání - "STELLAR ATMOSPHERES"
-
1
Influence of Collisions with Hydrogen Atoms on Non-LTE Effects for K I and Ca II in Stellar Atmospheres
ISSN: 1063-7737, 1562-6873Vydáno: Moscow Pleiades Publishing 01.09.2020Vydáno v Astronomy letters (01.09.2020)“… In agreement with the non-LTE studies available in the literature, K I is subject to overrecombination, which leads to a strengthening…”
Získat plný text
Journal Article -
2
How Hospitable Are Space Weather Affected Habitable Zones? The Role of Ion Escape
ISSN: 2041-8205, 2041-8213Vydáno: Goddard Space Flight Center The American Astronomical Society 10.02.2017Vydáno v Astrophysical journal. Letters (10.02.2017)“…Atmospheres of exoplanets in the habitable zones around active young G-K-M stars are subject to extreme X-ray and EUV (XUV…”
Získat plný text
Journal Article -
3
Measuring and Replicating the 1–20 μm Energy Distributions of the Coldest Brown Dwarfs: Rotating, Turbulent, and Nonadiabatic Atmospheres
ISSN: 0004-637X, 1538-4357Vydáno: Philadelphia The American Astronomical Society 01.09.2021Vydáno v The Astrophysical journal (01.09.2021)“…Cold, low-mass, field brown dwarfs are important for constraining the terminus of the stellar mass function, and also for optimizing atmospheric studies of…”
Získat plný text
Journal Article -
4
TRANSMISSION SPECTROSCOPY OF THE HOT JUPITER WASP-12b FROM 0.7 TO 5 μm
ISSN: 0004-6256, 1538-3881, 1538-3881Vydáno: United States 01.06.2014Vydáno v The Astronomical journal (01.06.2014)“…Since the first report of a potentially non-solar carbon-to-oxygen ratio (C/O) in its dayside atmosphere, the highly irradiated exoplanet WASP-12b has been under intense scrutiny and the subject of many follow-up observations…”
Získat plný text
Journal Article -
5
XUV-driven mass loss from extrasolar giant planets orbiting active stars
ISSN: 0019-1035, 1090-2643Vydáno: Elsevier Inc 01.04.2015Vydáno v Icarus (New York, N.Y. 1962) (01.04.2015)“…•EGPs around more active stars have stability limit at larger orbital distances. Upper atmospheres of Hot Jupiters are subject to extreme radiation conditions that can result in rapid atmospheric escape…”
Získat plný text
Journal Article -
6
Investigating Non-LTE Abundances of Neodymium in Metal-poor FGK Stars
ISSN: 0004-637X, 1538-4357, 1538-4357Vydáno: Philadelphia The American Astronomical Society 20.11.2025Vydáno v The Astrophysical journal (20.11.2025)“…The dominant site(s) of the r-process are a subject of current debate. Ejecta from r-process-enrichment events like kilonovae are difficult to directly measure…”
Získat plný text
Journal Article -
7
FORMATION OF SOLAR FILAMENTS BY STEADY AND NONSTEADY CHROMOSPHERIC HEATING
ISSN: 0004-637X, 1538-4357Vydáno: United States 10.08.2011Vydáno v The Astrophysical journal (10.08.2011)“…It has been established that cold plasma condensations can form in a magnetic loop subject to localized heating of its footpoints…”
Získat plný text
Journal Article -
8
Deconstructing Photospheric Spectral Lines in Solar and Stellar Flares
ISSN: 0004-637X, 1538-4357Vydáno: Philadelphia The American Astronomical Society 01.03.2024Vydáno v The Astrophysical journal (01.03.2024)“…/stellar atmosphere to electron beam heating and synthesize spectral lines of Fe i to investigate the line…”
Získat plný text
Journal Article -
9
Photoionization of Atoms
ISBN: 3725826722, 9783725826728, 9783725826711, 3725826714Vydáno: Basel MDPI - Multidisciplinary Digital Publishing Institute 2024“…Photoionization is a process of ionization by photons. It is one of the most important processes for studying astronomical objects. This Special Issue will…”
Získat plný text
E-kniha -
10
THE EFFECTS OF THE IONOSPHERE ON GROUND-BASED DETECTION OF THE GLOBAL 21 cm SIGNAL FROM THE COSMIC DAWN AND THE DARK AGES
ISSN: 0004-637X, 1538-4357Vydáno: Philadelphia The American Astronomical Society 01.11.2016Vydáno v The Astrophysical journal (01.11.2016)“…ABSTRACT Detection of the global H i 21 cm signal from the Cosmic Dawn and the Epoch of Reionization is the key science driver for several ongoing ground-based…”
Získat plný text
Journal Article -
11
Direct Observation of the Radial Magnetic Field Gradient in HD 58260 from Spectropolarimetry of NLTE Lines in Emission
ISSN: 0004-637X, 1538-4357Vydáno: Philadelphia The American Astronomical Society 01.01.2022Vydáno v The Astrophysical journal (01.01.2022)“…Because of the unquestionable presence of magnetic fields in stars, their role in the structure of stellar atmospheres has for a long time been a subject of speculation…”
Získat plný text
Journal Article -
12
On the formation of super-Jupiters: core accretion or gravitational instability?
ISSN: 0004-640X, 1572-946XVydáno: Dordrecht Springer Netherlands 01.12.2024Vydáno v Astrophysics and space science (01.12.2024)“… However, the formation of super-massive planets remains a subject of debate, as their formation via the Core Accretion model requires super-solar metallicities…”
Získat plný text
Journal Article -
13
COMMISSION 36: THEORY OF STELLAR ATMOSPHERES
ISSN: 1743-9213, 1743-9221Vydáno: Cambridge, UK Cambridge University Press 01.12.2008Vydáno v Proceedings of the International Astronomical Union (01.12.2008)“…Commission 36 covers the whole field of the physics of stellar atmospheres. The scientific activity in this large subject has been very intense during the last…”
Získat plný text
Journal Article -
14
Numerical Modeling of Footpoint-driven Magneto-acoustic Wave Propagation in a Localized Solar Flux Tube
ISSN: 0004-637X, 1538-4357Vydáno: United States IOP Publishing 20.01.2011Vydáno v The Astrophysical journal (20.01.2011)“…In this paper, we present and discuss results of two-dimensional simulations of linear and nonlinear magneto-acoustic wave propagation through an open magnetic…”
Získat plný text
Journal Article -
15
A Reconnecting Current Sheet Imaged in a Solar Flare
ISSN: 2041-8205, 2041-8213Vydáno: United States IOP Publishing 01.11.2010Vydáno v Astrophysical journal. Letters (01.11.2010)“… For flares and coronal mass ejections (CMEs) in the solar atmosphere, the standard model predicts the presence of a reconnecting current sheet, which has been the subject of considerable theoretical and numerical modeling over the last 50 years…”
Získat plný text
Journal Article -
16
VERTICAL STRUCTURE OF MAGNETIZED ACCRETION DISKS AROUND YOUNG STARS
ISSN: 0004-637X, 1538-4357Vydáno: United Kingdom The American Astronomical Society 20.01.2016Vydáno v The Astrophysical journal (20.01.2016)“…ABSTRACT We model the vertical structure of the magnetized accretion disks that are subject to viscous and resistive heating and irradiation by the central star…”
Získat plný text
Journal Article -
17
SPECTROSCOPIC METALLICITY DETERMINATIONS FOR W UMa-TYPE BINARY STARS
ISSN: 0004-6256, 1538-3881, 1538-3881Vydáno: United States 01.09.2013Vydáno v The Astronomical journal (01.09.2013)“… relatively low quality of the data, all spectra were subject to the same broadening function (BF) processing to determine the combined line strength in the spectral window centered on the Mg I triplet between 5080 A and 5285…”
Získat plný text
Journal Article -
18
The Role Of Torsional Alfvén Waves in Coronal Heating
ISSN: 0004-637X, 1538-4357Vydáno: Bristol IOP Publishing 20.03.2010Vydáno v The Astrophysical journal (20.03.2010)“…In the context of coronal heating, among the zoo of magnetohydrodynamic (MHD) waves that exist in the solar atmosphere, Alfven waves receive special attention…”
Získat plný text
Journal Article -
19
NON-AXISYMMETRIC FLOWS ON HOT JUPITERS WITH OBLIQUE MAGNETIC FIELDS
ISSN: 1538-4357, 0004-637X, 1538-4357Vydáno: United States 10.10.2014Vydáno v The Astrophysical journal (10.10.2014)“…Giant planets that reside in close proximity to their host stars are subject to extreme irradiation, which gives rise to thermal ionization of trace alkali metals in their atmospheres…”
Získat plný text
Journal Article -
20
NUMERICAL EXPERIMENTS ON THE TWO-STEP EMERGENCE OF TWISTED MAGNETIC FLUX TUBES IN THE SUN
ISSN: 0004-637X, 1538-4357Vydáno: Bristol IOP 10.07.2011Vydáno v The Astrophysical journal (10.07.2011)“… We find that the evolution is illustrated by the following two-step process. The initial tube rises due to its buoyancy, subject to aerodynamic drag due to the external flow…”
Získat plný text
Journal Article

