Results 1 to 10 of about 2,636,588 (34)

3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR 3. II. Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures [PDF]

open access: yesAstrophysical Journal, 2022
We identify members of 65 open clusters in the solar neighborhood using the machine-learning algorithm StarGO based on Gaia EDR3 data. After adding members of 20 clusters from previous studies we obtain 85 clusters, and study their morphology and ...
X. Pang   +26 more
semanticscholar   +1 more source

The Palomar Transient Factory Core-collapse Supernova Host-galaxy Sample. I. Host-galaxy Distribution Functions and Environment Dependence of Core-collapse Supernovae [PDF]

open access: yesAstrophysical Journal Supplement Series, 2020
Several thousand core-collapse supernovae (CCSNe) of different flavors have been discovered so far. However, identifying their progenitors has remained an outstanding open question in astrophysics.
S. Schulze   +56 more
semanticscholar   +1 more source

NGTS-10b: the shortest period hot Jupiter yet discovered [PDF]

open access: yesMonthly notices of the Royal Astronomical Society, 2019
We report the discovery of a new ultrashort period (USP) transiting hot Jupiter from the Next Generation Transit Survey (NGTS). NGTS-10b has a mass and radius of $2.162\, ^{+0.092}_{-0.107}$ MJ and $1.205\, ^{+0.117}_{-0.083}$ RJ and orbits its host ...
J. McCormac   +101 more
semanticscholar   +1 more source

Stellar laboratories: new Ge V and Ge VI oscillator strengths and their validation in the hot white dwarf RE 0503–289 [PDF]

open access: yes, 2012
Context. State-of-the-art spectral analysis of hot stars by means of non-LTE model-atmosphere techniques has arrived at a high level of sophistication. The analysis of high-resolution and high-S/N spectra, however, is strongly restricted by the lack of ...
T. Rauch   +22 more
semanticscholar   +1 more source

The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards - I. NLTE spectral analysis of the DA-type white dwarf G191−B2B [PDF]

open access: yes, 2013
Hydrogen-rich, DA-type white dwarfs are particularly suited as primary standard stars for flux calibration. State-of-the-art NLTE models consider opacities of species up to trans-iron elements and provide reliable synthetic stellar-atmosphere spectra to ...
T. Rauch   +15 more
semanticscholar   +1 more source

Circumstellar discs in Galactic centre clusters: Disc-bearing B-type stars in the Quintuplet and Arches clusters [PDF]

open access: yes, 2015
Astronomy & Astrophysics manuscript no. discs_astro_11feb2014 February 13, 2015 c ESO Circumstellar discs in Galactic centre clusters: Disc-bearing B-type stars in the Quintuplet and Arches clusters ? A. Stolte 1 , B. Husmann 1 , C.
A. Stolte   +9 more
semanticscholar   +1 more source

BD–22°3467, a DAO-type star exciting the nebula Abell 35 [PDF]

open access: yes, 2012
Context. Spectral analyses of hot, compact stars with non-local thermodynamical equilibrium (NLTE) model-atmosphere techniques allow the precise determination of photospheric parameters such as the effective temperature (Teff), the surface gravity (log g)
M. Ziegler   +18 more
semanticscholar   +1 more source

Coronal Abundances in Orion Nebula Cluster Stars [PDF]

open access: yes, 2007
Following the Chandra Orion Ultradeep Project (COUP) observation, we have studied the chemical composition of the hot plasma in a sample of 146 X-ray-bright pre-main-sequence stars in the Orion Nebula Cluster (ONC).
A. Maggio   +9 more
semanticscholar   +1 more source

Linear Solar Models: a simple tool to investigate the properties of solar interior [PDF]

open access: yes, 2010
We describe a simple method to study the dependence of the solar properties on a generic (small) modification the physical inputs adopted in standard solar models calculations.
arxiv   +1 more source

Helicity--vorticity turbulent pumping of magnetic fields in the solar dynamo [PDF]

open access: yes, 2012
The interaction of helical convective motions and differential rotation in the solar convection zone results in turbulent drift of a large-scale magnetic field. We discuss the pumping mechanism and its impact on the solar dynamo.
arxiv   +1 more source

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