AAVSO Alert Notice 412 Nova Sct 2009 (V496 Sct) November 10, 2009 Event: Nova in Scutum (V496 Sct == N Sct 2009) Discovered By: H. Nishimura (Miyawaki, Kakegawa, Japan) Discovery Date: 2009 November 8.370 UT Discovery Magnitude: unfiltered CCD magnitude of 8.8, using 120-mm camera lens, derived by S. Nakano (Sumoto, Japan) from Nishimura's discovery images. Position: RA: 18:43:45.57 , Dec: -7:36:42.0 (equinox 2000.0) from E. Guido and G. Sostero, using a 0.25-m reflector sited at Mayhill, New Mexico, USA. Spectra: A low-resolution spectrum was obtained by F. Teyssier using a 0.2-meter telescope equipped with a spectrograph having an effective resolution of 8.56 Angstroms (4.28 Angstroms/pixel, 2-pixel bins). This spectrum clearly shows the presence of the H-alpha and H-beta lines, both having P Cygni profiles. Several weaker emission lines are also present. D. Balam (NRCC) and G. Sarty (U. Sask.) obtained a spectrum covering the wavelength range of 429-455 nanometers on 2009 November 10.08 UT confirming the presence of several emission lines having P Cygni profiles. U. Munari et al. (INA-Padova & the Asiago Novae and Symbiotic Stars Collaboration) report a low-resolution spectrum (0.21 nm/pix) obtained on 2009 November 9.779 UT with a 0.6-meter telescope. The spectrum contains multiple emission lines including the H-Balmer series, OI, and FeII, all with P Cygni profiles. The presence of FeII lines indicates a nova of the Fe II-type. Observations Reported to the AAVSO: 2009 Nov 9.0932 (JD 2455144.5932), R=7.76 (V. Mechinsky, Minsk, Belarus); Nov 9.7549 (2455145.2549), m(vis)=8.4 (S. Shaffer, Laramie, Wyoming, USA); Nov 9.8717 (2455145.3717), CV=8.61 (C. Spratt, Victoria, B.C., Canada); Nov 10.0506 (2455145.5506), V=8.04 (S. Howerton, Arkansas City, Kansas, USA); Nov 10.0625 (2455145.5625), m(vis)=8.4 (S. Aguirre, Hermosillo, Sonora, Mexico). Charts: Finder charts for V496 Sct may be plotted by entering the coordinates above into VSP: http://www.aavso.org/observing/charts/vsp/ Reporting Observations: Please report all observations to the AAVSO as "V496 Sct". The names "Nova Sct 2009" or "VSX J184345.5-073642" are equivalent, but the GCVS name is preferred. Notes: a. The object was initially announced in CBET #2008 (D.W.E. Green, editor), where the discoverer notes that no object was visible on an image taken on 2009 November 7.377 using the same camera, with a limiting magnitude of 11.5 (unfiltered). b. E. Guido and G. Sostero reported their confirmation and improved position in CBET #2008, with images taken with the GRAS 0.25-m telescope sited near Mayhill, NM on 2009 November 9.08. Guido and Sostero also note that no unambiguous progenitor appears on a red DSS plate taken on 1996 August 13. c. F. Teyssier (Rouen, France) kindly provided a spectrum of the object taken on 2009 November 9.729 indicating the presence of Hydrogen and other emission lines with P Cygni profiles. An image of this spectrum may be obtained from the following website: http://www.astronomie-amateur.fr/Projets%20Spectro4%20Novae.html d. Information on name assignment and spectroscopic information used in this Alert Notice were taken from IAU Circular #9093 (D.W.E. Green, editor). This Alert Notice supersedes AAVSO Special Notice #176 (2009 November 9). Congratulations to H. Nishimura for his discovery! Good observing, Matthew Templeton, AAVSO