Nova Nor 2005 [V382 Nor]
Abstract:
The nova appears dominated by very strong H-alpha emission. Low-ionization emissions lines from Fe II (multiplets 27, 28, 37, 38, 42, 48, 49, and 74) and Na I are clearly visible. The Balmer and Fe II lines are flanked by weak P-Cyg profiles that indicate an average expansion velocity of 1100 +/- 100 km/s. The Na I interstellar lines appear saturated, thus suggesting a high absorption/reddening.
Justification:
Observation of nova V382 Nor to study its properties including emission lines and expansion velocity.
Requested Data Types:
Photometry, Spectroscopy
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| R Nor | 6.50 | M |
Cadence: Not Specified Precision: 100 |
Cadence: Not Specified Resolution: 250 Desired SNR: 100 |
Spectroscopy Lines:
Sodium Doublet (5890.0 Å), H-alpha (6563.0 Å)
Photometry Filters:
B (Johnson), V (Johnson), r (Sloan)
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: William Liller; Imported Campaign (Alert Notice #315)