We present a search for 12CO and SiO emission in V838 Mon. We derive upper limits on the 12CO and SiO emission, and on the total mass of the circumstellar material. Using an excitation temperature of 1000 K, and a likely distance of 6 kpc, the non-detection of 12CO emission leads to a 3σ upper limit on the mass of gas around the central star to be 10-2 $M_{\odot}$.
The asymptotic giant branch (AGB) is part of the late evolution of stars with initial masses of 0.8-...
We carried out 12CO(1−0) and 12CO(2−1) observations of 21 different regions in the vicinity of M 8...
Aims. HESS J1858+020 is a weak γ-ray source lying near the southern border of the SNR G35.6-0.4. A m...
We present a search for 12CO and SiO emission in V838 Mon. We derive upper limits on the 12CO and Si...
Aims. We aim to probe the close and distant circumstellar environments of the stellar outburst objec...
Aims. We aim to probe the close and distant circumstellar environments of the stellar outb...
Context. V838 Mon erupted at the beginning of 2002, becoming an extremely luminous star with L = 10...
The central region of the Monoceros R2 molecular cloud has been studied using molecular line maps, m...
We have detected emission in the J = 6 → 5 transition (λ = 453 µm) of the carbon monoxide isotopolog...
Context. The [C II] 158 μm line is one of the dominant coolants of the ISM, and an important probe w...
Aims. We investigate the suitability of several molecular tracers, in particular CN N = 2−1 line emi...
Artículo de publicación ISIWe report the detection of the SiO (J = 2−1) transition from the massive ...
Detecting molecular line emission from classical nova remnants has the potential to reveal informati...
Aims. We investigate the physical properties and spatial distribution of Carbon Monoxide (CO) gas in...
We present ISO Short-Wavelength Spectrometer observations of pure-rotational line emissionH2from the...
The asymptotic giant branch (AGB) is part of the late evolution of stars with initial masses of 0.8-...
We carried out 12CO(1−0) and 12CO(2−1) observations of 21 different regions in the vicinity of M 8...
Aims. HESS J1858+020 is a weak γ-ray source lying near the southern border of the SNR G35.6-0.4. A m...
We present a search for 12CO and SiO emission in V838 Mon. We derive upper limits on the 12CO and Si...
Aims. We aim to probe the close and distant circumstellar environments of the stellar outburst objec...
Aims. We aim to probe the close and distant circumstellar environments of the stellar outb...
Context. V838 Mon erupted at the beginning of 2002, becoming an extremely luminous star with L = 10...
The central region of the Monoceros R2 molecular cloud has been studied using molecular line maps, m...
We have detected emission in the J = 6 → 5 transition (λ = 453 µm) of the carbon monoxide isotopolog...
Context. The [C II] 158 μm line is one of the dominant coolants of the ISM, and an important probe w...
Aims. We investigate the suitability of several molecular tracers, in particular CN N = 2−1 line emi...
Artículo de publicación ISIWe report the detection of the SiO (J = 2−1) transition from the massive ...
Detecting molecular line emission from classical nova remnants has the potential to reveal informati...
Aims. We investigate the physical properties and spatial distribution of Carbon Monoxide (CO) gas in...
We present ISO Short-Wavelength Spectrometer observations of pure-rotational line emissionH2from the...
The asymptotic giant branch (AGB) is part of the late evolution of stars with initial masses of 0.8-...
We carried out 12CO(1−0) and 12CO(2−1) observations of 21 different regions in the vicinity of M 8...
Aims. HESS J1858+020 is a weak γ-ray source lying near the southern border of the SNR G35.6-0.4. A m...