Clues to Substellar Formation: Rotation and the Low-Mass End of the Initial Mass Function     

María Rosa Zapatero Osorio  José Caballero  Eduardo L. Martín  Víctor J.S. Béjar  Rafael Rebolo 《Astrophysics and Space Science》2004,292(1-4):673-679

We have monitored S Ori 45, a young, low-mass (20 M _j up) brown dwarf of the σ Orionis cluster (～3 Myr, 352 pc), using optical and near-infrared filters. S Ori 45 (spectral type M8.5) is found to be multi-periodic with a dominant modulation at 2.5–3.5 h, and a short modulation at about 46 min. We ascribe the longer of these modulations to a rotation period. After comparing these results with observations of more massive cluster brown dwarfs and field brown dwarfs, we conclude that substellar objects present rotational and angular momentum evolution. We have also obtained intermediate-resolution near-infrared spectroscopy of S Ori 70, which is a T-class, free-floating planetary candidate member in the σ Orionis cluster. Its observed spectrum has been compared to data of field brown dwarfs of similar types and to theoretical spectra computed for different surface temperatures and gravities. We conclude that S Ori 70 has a significantly cool, low-gravity atmosphere. This supports the young age of this object and its membership in the cluster. From state-of-the-art evolutionary models, the mass of S Ori 70 is estimated at 3 times the Jovian mass (⁺⁵ _?2 M _j up), challenging current stellar/substellar formation models. S Ori 70 remains the lowest mass object so far identified in any open cluster.  相似文献   

Rapid finite-fault analysis of large Mexico earthquakes using teleseismic P waves     

Mendoza  C.  Martínez-López  M. R. 《Journal of Seismology》2022,26(2):333-342

Journal of Seismology - We propose a rapid, finite-fault inversion procedure to derive first-order estimates of the coseismic slip following large Mw > 7 earthquakes in Mexico using...  相似文献   

Climate change influence on runoff and soil losses in a rainfed basin with Mediterranean climate   总被引：2，自引：2，他引：0  

M. C. Ramos  J. A. Martínez-Casasnovas 《Natural Hazards》2015,78(2):1065-1089

  相似文献   

Volcanism–sedimentation interaction in the Campo de Calatrava Volcanic Field (Spain): a magnetostratigraphic and geochronological study     

Antonio Herrero-Hernández  Francisco Javier López-Moro  José Luis Gallardo-Millán  Ángel Martín-Serrano  Fernando Gómez-Fernández 《International Journal of Earth Sciences》2015,104(1):103-122

  相似文献   

Numerical continuation of families of frozen orbits in the zonal problem of artificial satellite theory     

Martín Lara  André Deprit  Antonio Elipe 《Celestial Mechanics and Dynamical Astronomy》1995,62(2):167-181

In the zonal problem of a satellite around the Earth, we continue numerically natural families of periodic orbits with the polar component of the angular momentum as the parameter. We found three families; two of them are made of orbits with linear stability while the third one is made of unstable orbits. Except in a neighborhood of the critical inclination, the stable periodic (or frozen) orbits have very small eccentricities even for large inclinations.  相似文献   

Classical T Tauri Stars and Substellar Analogs     

D. Barrado Y Navascués  E.L. Martín  R. Jayawardhana  S. Mohanty 《Astrophysics and Space Science》2004,292(1-4):665-672

We propose a spectroscopic criterion based on Hα equivalent width and spectral type to classify classical T Tauri stars and substellar analogs. We argue that accreting objects can be identified from low-resolution optical spectroscopy, when their Hα flux is stronger than the saturation limit at Log {Lum(Hα)/Lum(bol)} = ?3.3. Additional criteria, such as the relation between HeI5876 or HeI6678 and Hα, or the ratios between the components of the CaII infrared triplet, are also discussed. We have tested the reliability of these criteria by applying them to several objects with masses in the range 0.11–0.025 M_⊙, which belong to nearby star forming regions and the TW Hya association.  相似文献   

Behaviour of the SMF method for the numerical integration of satellite orbits     

Pablo Martín  José M. Ferrándiz 《Celestial Mechanics and Dynamical Astronomy》1995,63(1):29-40

The SMF algorithms were recently developed by the authors as a multistep generalization of the ScheifeleG-functions one-step method. Like the last, the proposed codes integrate harmonic oscillations without truncation error and the perturbing parameter appears as a factor of that error when integrating perturbed oscillations. Therefore they seemed to be convenient for the accurate integration of orbital problems after the application of linearizing transformations, such as KS or BF. In this paper we present several numerical experiments concerning the propagation of Earth satellite orbits, that illustrate the performance of the the SMF method. In general, it provides greater accuracy than the usual standard algorithms for similar computational cost.  相似文献   

The ionized gas in the Galactic Center Radio Arc     

N.J. RodrÍguez-Fernández  J. MartÍn-Pintado  P. de Vicente 《Astrophysics and Space Science》2002,281(1-2):333-334

  相似文献   

Improved Approximated Solutions to the Nonlinear Debye Potential     

R.J. Pérez  P. Martín 《Astrophysics and Space Science》1997,256(1-2):263-268

The shielding effect of plasma on the electrostatic potential due to a central nucleus is studied. The potential is determined by the Poisson equation with Boltzmann factor for the charge density of ions. The aim of this work is to find approximated analytical solutions, without the usual linearization hypothesis, by means of the technique of quasifractional approximants in two points. In a previous work (Martín and Pérez, 1994) a quasifractional fractional approximation was obtained, but the coefficients were found by means of the numerical solution of the differential equation. Now we find a complete analytical expression. The approximant found is highly precise in the range of validity of the physical model used.  相似文献   

Space Charge Potentials in Cylindrical Geometries Including Temperature Effects     

E. Valdeblanquez  P. Martín 《Astrophysics and Space Science》1997,256(1-2):369-372

The analysis of space-charge in cylindrical geometries has been performed using kinetic theory. The current collected by central electrodes inmersed in plasmas with a discriminant grid has been determined through the Poisson equation and truncated Maxwellian distribution functions for the ions. The electrons are assumed to be repelled by the entrance grid. The non-linear adimensional equations have been solved approximately using linear expansion around the point with zero potential.  相似文献