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

^*Awdur cyfatebol y gwaith hwn

Cyfadran Cyfrifiadureg, Peirianneg a Gwyddoniaeth

Allbwn ymchwil: Cyfraniad at gyfnodolyn › Erthygl › adolygiad gan gymheiriaid

2 Dyfyniadau (Scopus)

Crynodeb

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.

Iaith wreiddiol	Saesneg
Tudalennau (o-i)	227-235
Nifer y tudalennau	9
Cyfnodolyn	Astrophysics and Space Science
Cyfrol	255
Rhif cyhoeddi	1-2
Dynodwyr Gwrthrych Digidol (DOIs)	https://doi.org/10.1007/978-94-011-5076-7_35
Statws	Cyhoeddwyd - 1997

Mynediad at Ddogfen

10.1007/978-94-011-5076-7_35Trwydded: CC BY-NC-ND

Dyfynnu hyn

@article{08e68719675c4682b628ef3e211a4123,

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",

year = "1997",

doi = "10.1007/978-94-011-5076-7_35",

language = "English",

volume = "255",

pages = "227--235",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

publisher = "Springer",

number = "1-2",

}

TY - JOUR

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

Crynodeb

Mynediad at Ddogfen

Ôl bys

Dyfynnu hyn