Nova Sct 2009 (V496 Sct)
Abstract:
A nova in Scutum, referred to as V496 Sct or N Sct 2009, was discovered on November 8, 2009. The nova exhibited an unfiltered CCD magnitude of 8.8 and showed several emission lines with P Cygni profiles, including the H-alpha and H-beta lines. It has been confirmed to be a Fe II-type nova.
Justification:
Nova Sct 2009 presents a unique opportunity to study a nova event with clear Fe II-type characteristics and several emission lines with P Cygni profiles, providing valuable data for the understanding of nova mechanisms.
Requested Data Types:
Photometry, Spectroscopy
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| BMAM-V496 | 18.80 | UG |
Cadence: Not Specified Precision: 100 |
Cadence: Not Specified Resolution: 250 Desired SNR: 100 |
Spectroscopy Lines:
No spectroscopy lines provided
Photometry Filters:
No photometry filters provided
Comparison Stars:
No comparison stars provided
Co-Authorship
Observers are not eligible for co-authorship.
Additional Observer Input:
Not provided
Additional Submission Location:
Not provided
Forum URL
N/A
Notes:
Principal Investigator: H. Nishimura (Miyawaki, Kakegawa, Japan); Imported Campaign (Alert Notice #412)