Observations of Nova Muscae with the WATCH Instrument

I. Yu. Lapshov; V. V. Dremin; R. A. Sunyaev; Søren Brandt; Niels Lund

Observations of Nova Muscae with the WATCH Instrument

I. Yu. Lapshov, V. V. Dremin, R. A. Sunyaev, Søren Brandt, Niels Lund

National Space Institute

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

Abstract

A new bright transient x-ray source was discovered by WATCH instrument on board GRANAT spacecraft on January 8, 1991. Maximum flux from the newly discovered source was 2 Crab units in 8-20 keV spectral band. During January 16-21 WATCH detected the dip in the light curve of the x-ray Nova. On January 16, 1991 the flux decreased to half that of the Crab. In five days the source became brighter again. Light curves in two energy bands are presented.

Original language	English
Title of host publication	Proceedings of the Workshop on Nova Muscae 1991 : Lyngby, May 14-16 1991
Editors	Søren Brandt
Place of Publication	Lyngby
Publisher	Danish Space Research Institute
Publication date	1991
Pages	11-17
Publication status	Published - 1991
Event	Workshop on Nova Muscae 1991 - Lyngby, Denmark Duration: 14 May 1991 → 16 May 1991

Workshop

Workshop	Workshop on Nova Muscae 1991
Country	Denmark
City	Lyngby
Period	14/05/1991 → 16/05/1991

Series	DRI Report
Number	2
Volume	91
ISSN	0109-6605

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1 Participating in or organising a conference

Workshop on Nova Muscae 1991
Søren Brandt (Organizer)
14 May 1991 → 16 May 1991
Activity: Attending an event › Participating in or organising a conference

Cite this

@inproceedings{43ac1f7d504b4bebb272bf31f1c91b14,

title = "Observations of Nova Muscae with the WATCH Instrument",

abstract = "A new bright transient x-ray source was discovered by WATCH instrument on board GRANAT spacecraft on January 8, 1991. Maximum flux from the newly discovered source was 2 Crab units in 8-20 keV spectral band. During January 16-21 WATCH detected the dip in the light curve of the x-ray Nova. On January 16, 1991 the flux decreased to half that of the Crab. In five days the source became brighter again. Light curves in two energy bands are presented.",

author = "Lapshov, {I. Yu.} and Dremin, {V. V.} and Sunyaev, {R. A.} and S{\o}ren Brandt and Niels Lund",

year = "1991",

language = "English",

series = "DRI Report",

publisher = "Danish Space Research Institute",

number = "2",

pages = "11--17",

editor = "S{\o}ren Brandt",

booktitle = "Proceedings of the Workshop on Nova Muscae 1991",

note = "Workshop on Nova Muscae 1991 ; Conference date: 14-05-1991 Through 16-05-1991",

}

Observations of Nova Muscae with the WATCH Instrument. / Lapshov, I. Yu.; Dremin, V. V.; Sunyaev, R. A.; Brandt, Søren ; Lund, Niels.

Proceedings of the Workshop on Nova Muscae 1991: Lyngby, May 14-16 1991. ed. / Søren Brandt. Lyngby : Danish Space Research Institute, 1991. p. 11-17 (DRI Report; No. 2, Vol. 91).

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

TY - GEN

T1 - Observations of Nova Muscae with the WATCH Instrument

AU - Lapshov, I. Yu.

AU - Dremin, V. V.

AU - Sunyaev, R. A.

AU - Brandt, Søren

AU - Lund, Niels

PY - 1991

Y1 - 1991

N2 - A new bright transient x-ray source was discovered by WATCH instrument on board GRANAT spacecraft on January 8, 1991. Maximum flux from the newly discovered source was 2 Crab units in 8-20 keV spectral band. During January 16-21 WATCH detected the dip in the light curve of the x-ray Nova. On January 16, 1991 the flux decreased to half that of the Crab. In five days the source became brighter again. Light curves in two energy bands are presented.

AB - A new bright transient x-ray source was discovered by WATCH instrument on board GRANAT spacecraft on January 8, 1991. Maximum flux from the newly discovered source was 2 Crab units in 8-20 keV spectral band. During January 16-21 WATCH detected the dip in the light curve of the x-ray Nova. On January 16, 1991 the flux decreased to half that of the Crab. In five days the source became brighter again. Light curves in two energy bands are presented.

M3 - Article in proceedings

T3 - DRI Report

SP - 11

EP - 17

BT - Proceedings of the Workshop on Nova Muscae 1991

A2 - Brandt, Søren

PB - Danish Space Research Institute

CY - Lyngby

T2 - Workshop on Nova Muscae 1991

Y2 - 14 May 1991 through 16 May 1991

ER -