Detection of the thermal radio continuum emission from the G9.62+0.19-F Hot Core
We present new high resolution and high sensitivity multi-frequency VLA radio continuum observations of the G9.62+0.19-F hot molecular core. We
34 indexed results
We present new high resolution and high sensitivity multi-frequency VLA radio continuum observations of the G9.62+0.19-F hot molecular core. We
Sakurai's object is a born again AGB star of the very late thermal pulse flavor. In this contribution I will
As a progenitor of NHE (Non High Energy) GRBs, we propose a (C+O) star and a neutron star (black hole)
We present models of photometric evolution of galaxies in which the effects of a dusty interstellar medium have been included
We have investigated the formation of the binary radio pulsars PSR B2303+46 and PSR J1141-6545 via Monte Carlo simulations of
As discussed elsewhere in these proceedings, the double pulsar system is a magnificent laboratory for gravitational physics and for studying
The surface chemical composition of this remarkable star shows that it is hydrogen-deficient, carbon-rich and enriched in the light s-process
We report here on two complementary population synthesis studies which relate directly to the formation and evolution of neutron star
Infrared observations of the environment of the two Soft Gamma-ray Repeaters (SGRs) with the best known locations on the sky
We present recent results from our ongoing large scale variability survey of the Orion OB1 Association. In an area of
The conversion of the Crab pulsar wind from one dominated by Poynting flux close to the star to one dominated
We conjecture that the Sen-Seiberg limit of the Type IIA D2-brane action in a flat spacetime background can be resummed,
3EG J1835+5918 is the brightest of the so-called unidentified EGRET sources at intermediate galactic latitude (l,b)=(89,25). We obtained complete radio,
This review aims to give an overview of the contribution of the Hubble Space Telescope to our understanding of the
Hamiltonians whose symbols are not simply real valued, but matrix or, more generally, endomorphism valued functions appear in many places
HST is very well tailored for observations of extragalactic star clusters. One obvious reason is HST's high spatial resolution, but
We present the tidal tail distributions of a sample of candidate binary clusters located in the bar of the Large
A possible connection among host-galaxies of gamma-ray bursts, BL Lacs and quasars is analysed. It is believed that the gamma-ray
With the VLBA, we have observed water masers associated with the OH/IR star, W43A, which trace a birth and growth
It is known that in the WKB approximation of multicomponent systems like Dirac equation or Born-Oppenheimer approximation, an additional phase
We briefly discuss the evolutionary path and observational appearance of isolated neutron stars (INSs) focusing on radioquiet objects. There are
Marsden, Lingenfelter, Rothschild & Higdon have given arguments against the magnetar model for Soft Gamma Repeaters (SGRs) and Anomalous X-ray
We investigate the evolution of rigidly and differentially rotating protoneutron stars (PNSs) during the first twenty seconds of their life.
Precessing Gamma Jets, originated by Neutron Stars or Black Holes, may blaze to the observer leading to Gamma Bursts (GRBs)