One-electron molecular systems in a strong magnetic field
AV Turbiner, JCL Vieyra - Physics reports, 2006 - Elsevier
This review paper is inspired by a recent discovery by Chandra X-ray observatory of two
absorption features in the spectra of radiation of the isolated neutron star 1E1207. 4-5209 …
absorption features in the spectra of radiation of the isolated neutron star 1E1207. 4-5209 …
Modelling mid-Z element atmospheres for strongly magnetized neutron stars
K Mori, WCG Ho - Monthly Notices of the Royal Astronomical …, 2007 - academic.oup.com
We construct models for strongly magnetized neutron star atmospheres composed of mid-Z
elements (carbon, oxygen and neon) with magnetic fields B= 1012–1013 G and effective …
elements (carbon, oxygen and neon) with magnetic fields B= 1012–1013 G and effective …
Ultraviolet, X-ray, and optical radiation from the geminga pulsar
OY Kargaltsev, GG Pavlov, VE Zavlin… - The Astrophysical …, 2005 - iopscience.iop.org
We observed the γ-ray pulsar Geminga with the FUV-MAMA and NUV-MAMA detectors of
the Space Telescope Imaging Spectrometer to measure Geminga's spectrum and pulsations …
the Space Telescope Imaging Spectrometer to measure Geminga's spectrum and pulsations …
Detailed atmosphere modeling for the neutron star 1E1207. 4–5209: Evidence of oxygen/neon atmosphere
K Mori, CJ Hailey - The Astrophysical Journal, 2006 - iopscience.iop.org
We present a comprehensive investigation of the two broad absorption features observed in
the X-ray spectrum of the neutron star 1E1207. 4-5209 based on a recent analysis of the 260 …
the X-ray spectrum of the neutron star 1E1207. 4-5209 based on a recent analysis of the 260 …
Once-ionized helium in superstrong magnetic fields
GG Pavlov, VG Bezchastnov - The Astrophysical Journal, 2005 - iopscience.iop.org
It is generally believed that magnetic fields of some neutron stars, the so-called magnetars,
are enormously strong, up to 10 14-10 15 G. Recent investigations have shown that the …
are enormously strong, up to 10 14-10 15 G. Recent investigations have shown that the …
Detailed spectral analysis of the 260 ks XMM-Newton data of 1E 1207.4–5209 and significance of a 2.1 kev absorption feature
K Mori, JC Chonko, CJ Hailey - The Astrophysical Journal, 2005 - iopscience.iop.org
We have reanalyzed the 260 ks XMM-Newton observation of 1E 1207.4-5209. There are
several significant improvements over previous work. First, a much broader range of …
several significant improvements over previous work. First, a much broader range of …
Chemical Complexity and Prevalence of Life in the Universe: A New Method for the Estimation of Key Terms of Drake Equation
L Lamza - ar** our understanding of fundamental physics, including nuclear and particle physics …
Existence of the finite hydrogenic molecular chain and ion in a strong magnetic field
DJ Nader, JCL Vieyra, AV Turbiner - Physical Review A, 2019 - APS
The existence and stability of the linear hydrogenic chain H 3 and H 2− in a strong magnetic
field is established. Variational calculations for H 3 and H 2− are carried out in magnetic …
field is established. Variational calculations for H 3 and H 2− are carried out in magnetic …