The discovery of broad emission features between 3.2 and 3.6 microns were reported in the spectrum of Nova Cen 1986 (V842 Cen) some 300 days following outburst and remaining prominent for several months. The general characteristics of these features are similar to those attributed to polycyclic hydrocarbon (PAH) molecules in other dusty sources, although the relative strengths are different, and these observations provide the first clear evidence for molecular constituents other than graphite particles in the ejecta of novae
The discovery that many classical novae produce detectable GeV $\gamma$-ray emission has raised the ...
We present new Herschel photometric and spectroscopic observations of Supernova 1987A, carried out i...
Context. Classical novae are thermonuclear explosions that take place in the envelopes of accreting ...
Novae are generally considered to be hot astronomical objects and show effective temperatures up to ...
Abstract. A classical nova outburst arises from a thermonuclear run-away in the hydrogen-rich materi...
Broad-band infrared observations of FH Ser (Nova Ser 1970) covering the period 40 to 529 days after ...
We present infrared spectroscopy of the nova V705 Cas (1993), obtained following the dust formation ...
We observed the oxygen-rich Large Magellanic Cloud (LMC) supernova remnant N132D (SNR 0525-69.6), us...
Large discrepancies are found between observational estimates and theoretical predictions when explo...
We review the properties of dust formed during classical nova eruptions and the Very Late Thermal Pu...
We present 5-28 μm SOFIA FORECAST spectroscopy complemented by panchromatic X-ray through infrared o...
A fraction of classical novae form dust during the early stages of their outbursts. The classical CO...
We present ground-based infrared photometry, JHK spectroscopy, and 5-28 micron SOFIA FORCAST spectro...
We observed the oxygen-rich Large Magellanic Cloud (LMC) supernova remnant N132D (SNR 0525-69.6), us...
We present ground-based infrared photometry, JHK spectroscopy, and 5–28 μm SOFIA FORCAST spectroscop...
The discovery that many classical novae produce detectable GeV $\gamma$-ray emission has raised the ...
We present new Herschel photometric and spectroscopic observations of Supernova 1987A, carried out i...
Context. Classical novae are thermonuclear explosions that take place in the envelopes of accreting ...
Novae are generally considered to be hot astronomical objects and show effective temperatures up to ...
Abstract. A classical nova outburst arises from a thermonuclear run-away in the hydrogen-rich materi...
Broad-band infrared observations of FH Ser (Nova Ser 1970) covering the period 40 to 529 days after ...
We present infrared spectroscopy of the nova V705 Cas (1993), obtained following the dust formation ...
We observed the oxygen-rich Large Magellanic Cloud (LMC) supernova remnant N132D (SNR 0525-69.6), us...
Large discrepancies are found between observational estimates and theoretical predictions when explo...
We review the properties of dust formed during classical nova eruptions and the Very Late Thermal Pu...
We present 5-28 μm SOFIA FORECAST spectroscopy complemented by panchromatic X-ray through infrared o...
A fraction of classical novae form dust during the early stages of their outbursts. The classical CO...
We present ground-based infrared photometry, JHK spectroscopy, and 5-28 micron SOFIA FORCAST spectro...
We observed the oxygen-rich Large Magellanic Cloud (LMC) supernova remnant N132D (SNR 0525-69.6), us...
We present ground-based infrared photometry, JHK spectroscopy, and 5–28 μm SOFIA FORCAST spectroscop...
The discovery that many classical novae produce detectable GeV $\gamma$-ray emission has raised the ...
We present new Herschel photometric and spectroscopic observations of Supernova 1987A, carried out i...
Context. Classical novae are thermonuclear explosions that take place in the envelopes of accreting ...