Five-year optical and near-infrared observations of the extremely slow nova V1280 Scorpii

Astronomy and Astrophysics

Volumn 543, Issue , 2012, Pages

  Naito, H ^a   Mizoguchi, S ^b   Arai, A ^c   Tajitsu, A ^d   Narusawa, S ^e   Yamanaka, M ^f   Fujii, M ^g   Iijima, T ^h   Kinugasa, K ⁱ   Kurita, M ^a   Nagayama, T ^a   Yamaoka, H ^j   Sadakane, K ^k  

^a NAGOYA UNIVERSITY   (Japan)

^b Sendai Astronomical Observatory   (Japan)

^c KYOTO SANGYO UNIVERSITY   (Japan)

^d NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^e Nishi Harima Astronomical Observatory   (Japan)

^f HIROSHIMA UNIVERSITY   (Japan)

^g Fujii Bisei Obsevatory   (Japan)

^h INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

ⁱ Gunma Astronomical Observatory   (Japan)

^j KYUSHU UNIVERSITY   (Japan)

^k OSAKA KYOIKU UNIVERSITY   (Japan)

more..

Author keywords

Novae, cataclysmic variables; Stars: abundances; Stars: distances; Stars: individual: V1280 Sco

Indexed keywords

CLASSICAL NOVAE; DUST FORMATION; EXPANSION VELOCITY; NEAR INFRARED; NOVAE , CATACLYSMIC VARIABLES; NUCLEAR BURNING; OPTICAL BANDS; RE-IGNITION; STARS: ABUNDANCES; STARS: DISTANCES; STARS: INDIVIDUAL; WHITE DWARFS;

DUST; INFRARED DEVICES; PHOTOMETRY; STARS;

SLOW LIGHT;

EID: 84863324644     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118315     Document Type: Article

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