ISO Observations of V1425 Aquillae

Details ISO Observations of V1425 Aquillae ISO Observations of V1425 Aquillae

May 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...194.8607l&link_type=abstract

American Astronomical Society, 194th AAS Meeting, #86.07; Bulletin of the American Astronomical Society, Vol. 31, p.976

Astronomy and Astrophysics

Astronomy

Scientific paper

We present observations of the classical nova V1425 Aquillae (Nova Aquillae 1995) over four epochs obtained with the ISO Short Wavelength Spectrometer (SWS). We identify the following lines that appeared at least once over the four observations: HI 20-11 lambda 15.8, [NeIII]lambda 15.5, [NeV]lambda 14.3, [NeV]lambda 24.3, and [OIV]lambda 25.9. In three of four epochs, both a [NeV] and the [OIV] line appear allowing time evolution of the O to Ne abundance ratio. Additionally, the HI line in one observation allows the absolute abundances of O and Ne to be determined. J.E.L. was supported by NASA.

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