Near IR, multi-epoch, spectroscopic and photometric observations of the enigmatic, eruptive variable V838 Mon in JHK bands are reported. One of the unusual features is the detection of several strong neutral TiI lines in emission in the K band. From the strength of these lines, the mass of the ejected envelope is estimated to be in the range 10e-7 to 10e-5 M(sun). The spectra also show the strong presence of the first and second overtones of 12CO bands seen in the K and H bands. The CO bands show a complex evolution. Deep water bands at 1.4 and 1.9 micron are also seen later in the object's evolution. Blackbody fits to the JHK photometric data show that V838 Mon has evolved to temperatures between 2400 - 2600 K by approximately 130 days aft...
Aims. V838 Monocerotis erupted in 2002, brightened in a series of outbursts, and eventually develope...
V838 Mon is the prototype of a new class of objects. Understanding the nature of its multi-stage out...
After four years during which only the spectacular light echo was showing continuous and rapid evolu...
Near – IR, multi – epoch, spectroscopic and photometric observations of the enigmatic, eruptive var...
We report optical and near-infrared spectroscopy, and optical spectropolarimetry, of the peculiar va...
We report spectra of the overtone and fundamental bands of CO in the eruptive variable V838 Mon, whi...
The eruptive variable V838 Monocerotis (V838 Mon) gained notoriety in 2002 when it brightened nine m...
We present the results of modelling the 0.45--1 micron spectral energy distribution of V838 Mon for ...
We present photometric and high- and low-resolution spectroscopic observations of the unusual outbur...
Context. V838 Mon erupted at the beginning of 2002. In the course of the outburst the object evolved...
International audienceAims. V838 Monocerotis erupted in 2002, brightened in a series of outbursts, a...
Aims. We aim to probe the close and distant circumstellar environments of the stellar outburst objec...
We describe the results of fitting simple spherically symmetric models to the first overtone CO and ...
The unusual variable star V838 Monocerotis underwent an eruption in 2002. It continues to illuminate...
We present Spitzer observations of the unusual variable V838 Monocerotis. Extended emission is detec...
Aims. V838 Monocerotis erupted in 2002, brightened in a series of outbursts, and eventually develope...
V838 Mon is the prototype of a new class of objects. Understanding the nature of its multi-stage out...
After four years during which only the spectacular light echo was showing continuous and rapid evolu...
Near – IR, multi – epoch, spectroscopic and photometric observations of the enigmatic, eruptive var...
We report optical and near-infrared spectroscopy, and optical spectropolarimetry, of the peculiar va...
We report spectra of the overtone and fundamental bands of CO in the eruptive variable V838 Mon, whi...
The eruptive variable V838 Monocerotis (V838 Mon) gained notoriety in 2002 when it brightened nine m...
We present the results of modelling the 0.45--1 micron spectral energy distribution of V838 Mon for ...
We present photometric and high- and low-resolution spectroscopic observations of the unusual outbur...
Context. V838 Mon erupted at the beginning of 2002. In the course of the outburst the object evolved...
International audienceAims. V838 Monocerotis erupted in 2002, brightened in a series of outbursts, a...
Aims. We aim to probe the close and distant circumstellar environments of the stellar outburst objec...
We describe the results of fitting simple spherically symmetric models to the first overtone CO and ...
The unusual variable star V838 Monocerotis underwent an eruption in 2002. It continues to illuminate...
We present Spitzer observations of the unusual variable V838 Monocerotis. Extended emission is detec...
Aims. V838 Monocerotis erupted in 2002, brightened in a series of outbursts, and eventually develope...
V838 Mon is the prototype of a new class of objects. Understanding the nature of its multi-stage out...
After four years during which only the spectacular light echo was showing continuous and rapid evolu...