ISO observations of classical novae: Preliminary analysis and results

A. Salama; P. Barr; J. Clavel; K. Leech; M. F. Kessler; T. Lim; L. Metcalfe; B. Schulz; S. P.S. Eyres; R. N.  Jenkins; A. Evans

doi:10.1007/978-94-011-5076-7_35

ISO observations of classical novae: Preliminary analysis and results

A. Salama^*, P. Barr, J. Clavel, K. Leech, M. F. Kessler, T. Lim, L. Metcalfe, B. Schulz, S. P.S. Eyres, R. N. Jenkins, A. Evans

^*Corresponding author for this work

Faculty of Computing, Engineering and Science

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2 Citations (Scopus)

Abstract

We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines are providing us with information about physical conditions in nova ejecta which complement and extend knowledge obtained from ground-based observations. Surprisingly, we are getting little information about dust in nova systems, despite the fact that many novae are prolific dust-producers.

Original language	English
Pages (from-to)	227-235
Number of pages	9
Journal	Astrophysics and Space Science
Volume	255
Issue number	1-2
DOIs	https://doi.org/10.1007/978-94-011-5076-7_35
Publication status	Published - 1997

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title = "ISO observations of classical novae: Preliminary analysis and results",

abstract = "We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines are providing us with information about physical conditions in nova ejecta which complement and extend knowledge obtained from ground-based observations. Surprisingly, we are getting little information about dust in nova systems, despite the fact that many novae are prolific dust-producers.",

author = "A. Salama and P. Barr and J. Clavel and K. Leech and Kessler, {M. F.} and T. Lim and L. Metcalfe and B. Schulz and Eyres, {S. P.S.} and Jenkins, {R. N.} and A. Evans",

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T1 - ISO observations of classical novae

T2 - Preliminary analysis and results

AU - Salama, A.

AU - Barr, P.

AU - Clavel, J.

AU - Leech, K.

AU - Kessler, M. F.

AU - Lim, T.

AU - Metcalfe, L.

AU - Schulz, B.

AU - Eyres, S. P.S.

AU - Jenkins, R. N.

AU - Evans, A.

PY - 1997

Y1 - 1997

N2 - We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines are providing us with information about physical conditions in nova ejecta which complement and extend knowledge obtained from ground-based observations. Surprisingly, we are getting little information about dust in nova systems, despite the fact that many novae are prolific dust-producers.

AB - We describe the ISO programme to observe classical novae. The programme includes observations of novae during and shortly after eruption, and old novae. ISO observations of far infrared fine structure lines are providing us with information about physical conditions in nova ejecta which complement and extend knowledge obtained from ground-based observations. Surprisingly, we are getting little information about dust in nova systems, despite the fact that many novae are prolific dust-producers.

U2 - 10.1007/978-94-011-5076-7_35

DO - 10.1007/978-94-011-5076-7_35

M3 - Article

AN - SCOPUS:2842561580

VL - 255

SP - 227

EP - 235

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

SN - 0004-640X

IS - 1-2

ER -

ISO observations of classical novae: Preliminary analysis and results

Abstract

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