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Statements

Subject Item
n2:RIV%2F00216305%3A26110%2F09%3APU85943%21RIV11-MSM-26110___
rdf:type
skos:Concept n15:Vysledek
dcterms:description
We discovered the first outburst of V455 And (=HS2331+3905) on Sep. 4 2007 at V=14.59, which has been considered a good candidate for the WZ Sge-type dwarf nova. A time-resolved photometry campaign was soon coordinated and covered the whole of the superoutburst from the rising phase to the slow fading tail. At the time of our outburst detection, the object was in the rising phase at a rate of 10 mag/day. We found that there were no orbital humps nor early superhumps during the rapid rising phase of superoutburst. Early superhumps with a period of 0.05626(1) days appeared around the maximum. Ordinary superhumps appeared 9 days after the maximum. The snperhump period was 0.057202(1) days which was 1.6 decline from the plateau 19 days after the maximum. After the rapid fading, the object showed a slow fading trend at a rate of 0.03 mag/day. During the early phase of the slow fading tail, superhumps with a period of 0.05728(3) days were observed. The object showed no rebrightenings. We will present the re We discovered the first outburst of V455 And (=HS2331+3905) on Sep. 4 2007 at V=14.59, which has been considered a good candidate for the WZ Sge-type dwarf nova. A time-resolved photometry campaign was soon coordinated and covered the whole of the superoutburst from the rising phase to the slow fading tail. At the time of our outburst detection, the object was in the rising phase at a rate of 10 mag/day. We found that there were no orbital humps nor early superhumps during the rapid rising phase of superoutburst. Early superhumps with a period of 0.05626(1) days appeared around the maximum. Ordinary superhumps appeared 9 days after the maximum. The snperhump period was 0.057202(1) days which was 1.6 decline from the plateau 19 days after the maximum. After the rapid fading, the object showed a slow fading trend at a rate of 0.03 mag/day. During the early phase of the slow fading tail, superhumps with a period of 0.05728(3) days were observed. The object showed no rebrightenings. We will present the re
dcterms:title
Photometric Observations of a WZ Sge-type Dwarf Nova V455 Andromedae during the 2007 Superoutburst Photometric Observations of a WZ Sge-type Dwarf Nova V455 Andromedae during the 2007 Superoutburst
skos:prefLabel
Photometric Observations of a WZ Sge-type Dwarf Nova V455 Andromedae during the 2007 Superoutburst Photometric Observations of a WZ Sge-type Dwarf Nova V455 Andromedae during the 2007 Superoutburst
skos:notation
RIV/00216305:26110/09:PU85943!RIV11-MSM-26110___
n3:aktivita
n14:S
n3:aktivity
S
n3:dodaniDat
n7:2011
n3:domaciTvurceVysledku
n12:2523205
n3:druhVysledku
n10:D
n3:duvernostUdaju
n19:S
n3:entitaPredkladatele
n16:predkladatel
n3:idSjednocenehoVysledku
333367
n3:idVysledku
RIV/00216305:26110/09:PU85943
n3:jazykVysledku
n11:eng
n3:klicovaSlova
EARLY SUPERHUMPS, URSAE-MAJORIS, HUMPS, STARS
n3:klicoveSlovo
n4:EARLY%20SUPERHUMPS n4:HUMPS n4:URSAE-MAJORIS n4:STARS
n3:kontrolniKodProRIV
[F7A019D6281C]
n3:mistoKonaniAkce
Phuket
n3:mistoVydani
SAN FRANCISCO
n3:nazevZdroje
EIGHTH PACIFIC RIM CONFERENCE ON STELLAR ASTROPHYSICS: A TRIBUTE TO KAM-CHING LEUNG
n3:obor
n6:BN
n3:pocetDomacichTvurcuVysledku
1
n3:pocetTvurcuVysledku
26
n3:rokUplatneniVysledku
n7:2009
n3:tvurceVysledku
Novák, Rudolf
n3:typAkce
n17:WRD
n3:wos
000271628900012
n3:zahajeniAkce
2008-05-05+02:00
s:numberOfPages
6
n13:hasPublisher
ASTRONOMICAL SOC PACIFIC
n8:isbn
978-1-58381-685-1
n20:organizacniJednotka
26110