ISO Observations of Classical Novae

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

ISO Observations of Classical Novae

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

Faculty of Computing, Engineering and Science

Research output: Chapter in Book/Report/Conference proceeding › Other chapter contribution › peer-review

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
Title of host publication	Astrophysics and Space Science
Editors	John Dyson, Susan A. Lamb, A. G. W. Cameron, A. M. Cherepashchuk, C.-G. Fälthammar, M. Kitamura, L. B. F. M. Waters, C. Waelkens, K. A. van der Hucht, P. A. Zaal
Publisher	Springer
Pages	227-235
ISBN (Electronic)	978-94-011-5076-7
ISBN (Print)	978-94-010-6132-2
Publication status	Published - 1998

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Salama, A., Barr, P., Clavel, J., Leech, K., Kessler, M. F., Lim, T., Metcalfe, L., Schulz, B., Eyres, S. P. S., Evans, A., & Jenkins, R. N. (1998). ISO Observations of Classical Novae. In J. Dyson, S. A. Lamb, A. G. W. Cameron, A. M. Cherepashchuk, C.-G. Fälthammar, M. Kitamura, L. B. F. M. Waters, C. Waelkens, K. A. van der Hucht, & P. A. Zaal (Eds.), Astrophysics and Space Science (pp. 227-235). Article Chapter 35 Springer.

@inbook{9fce27d22bc44508bdc75830b0a7d93e,

title = "ISO Observations of Classical Novae",

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 A. Evans and Jenkins, {R. N.}",

year = "1998",

language = "English",

isbn = "978-94-010-6132-2",

pages = "227--235",

editor = "John Dyson and Lamb, {Susan A.} and Cameron, {A. G. W.} and Cherepashchuk, {A. M.} and C.-G. F{\"a}lthammar and M. Kitamura and Waters, {L. B. F. M.} and C. Waelkens and {van der Hucht}, {K. A.} and Zaal, {P. A.}",

booktitle = "Astrophysics and Space Science",

publisher = "Springer",

address = "Germany",

}

Salama, A, Barr, P, Clavel, J, Leech, K, Kessler, MF, Lim, T, Metcalfe, L, Schulz, B, Eyres, SPS, Evans, A & Jenkins, RN 1998, ISO Observations of Classical Novae. in J Dyson, SA Lamb, AGW Cameron, AM Cherepashchuk, C-G Fälthammar, M Kitamura, LBFM Waters, C Waelkens, KA van der Hucht & PA Zaal (eds), Astrophysics and Space Science., Chapter 35, Springer, pp. 227-235.

ISO Observations of Classical Novae. / Salama, A.; Barr, P.; Clavel, J. et al.
Astrophysics and Space Science. ed. / John Dyson; Susan A. Lamb; A. G. W. Cameron; A. M. Cherepashchuk; C.-G. Fälthammar; M. Kitamura; L. B. F. M. Waters; C. Waelkens; K. A. van der Hucht; P. A. Zaal. Springer, 1998. p. 227-235 Chapter 35.

Research output: Chapter in Book/Report/Conference proceeding › Other chapter contribution › peer-review

TY - CHAP

T1 - ISO Observations of Classical Novae

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 - Evans, A.

AU - Jenkins, R. N.

PY - 1998

Y1 - 1998

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.

M3 - Other chapter contribution

SN - 978-94-010-6132-2

SP - 227

EP - 235

BT - Astrophysics and Space Science

A2 - Dyson, John

A2 - Lamb, Susan A.

A2 - Cameron, A. G. W.

A2 - Cherepashchuk, A. M.

A2 - Fälthammar, C.-G.

A2 - Kitamura, M.

A2 - Waters, L. B. F. M.

A2 - Waelkens, C.

A2 - van der Hucht, K. A.

A2 - Zaal, P. A.

PB - Springer

ER -

ISO Observations of Classical Novae

Abstract

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