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Alert Notice 544: 
Nova Scorpii 2016 = PNV J17381927-3725077

June 13, 2016

Event: Nova in Scorpius

Discovered by: Hideo Nishimura (Kakegawa, Shizuoka-ken, Japan) (reported by S. Nakano, Sumoto, Japan, via CBET 4285)

Discovery magnitude: 12.4 unfiltered CCD on three 10-s CCD frames, using a 200-mm-f.l. f/3.2 lens with a Canon EOS 5D digital camera

Discovery date: 2016 June 10.629 UT
 
Coordinates (2000.0): R.A. 17 38 19.31  Dec. -37 25 08.7   (from VSX)

Spectra (via CBET 4285): Spectroscopy obtained by K. Ayani (Bisei Astronomical Observatory, BAO) on 2016 Jun. 11.65 UT with the BAO 1.01-m telescope shows the star to be a nova in early stages. Ayani's spectrogram is posted at http://tinyurl.com/zqjkgjd.

Observing recommendations: Observations of all types (visual, CCD, DSLR, spectroscopy) as instrumentation permits are strongly encouraged as the nova evolves.

Charts: Charts for Nova Sco 2016 may be created using the AAVSO Variable Star Plotter (VSP). Be sure to include spaces in the name as shown.

Observations reported to the AAVSO:
2016 May 14.712 UT, <12.5 CCD (Nishimura; from CBET 4285);
18.602 <12.9 CCD (Nishimura; from CBET 4285);
Jun. 5.532, <13.0 CCD (Nishimura; from CBET 4285);
5.582, <13 CCD (T. Kojima, Gunma-ken, Japan; 135-mm-f.l. lens + Canon EOS 6D digital camera; from CBET 4285);
9.596, 11.8 CCD (Kojima; pre-discovery image found on three frames; from CBET 4285);
11.255, 12.36 V (S. Kiyota, Kamagaya, Japan, remotely with a 0.50-m f/4.5 CDK astrograph near Mayhill, NM, USA; from CBET 4285);
11.255, 11.42 Rc (Kiyota; from CBET 4285);
11.255, 10.00 Ic (Kiyota; from CBET 4285);
11.25716, 11.461 CV +/-0.004 (HMB, F.-J. Hambsch, Mol Belgium; selected from 30 V obs Jun 11.25716-11.37339);
11.31119, 11.396 CV +/-0.004 (Hambsch, as above);
11.37339, 11.397 CV +/-0.005 CV (Hambsch, as above);
11.506, 10.4 CCD (K. Itagaki, Yamagata, Japan, 0.50-m f/7.7 reflector at Tochigi station; from CBET 4285);
11.513, 11.3 CCD (T. Noguchi, Katori, Chiba-ken, Japan, 0.23-m f/6.3 Schmidt-Cassegrain reflector; from CBET 4285);
11.612, 10.95 R (F. Watanabe and H. Naito, Nayoro Observatory, 0.4-m Meili telescope; from CBET 4285);
11.63091, 11.2697 CV +/-0.0238 (SPET, P. Starr, Coonabarabran, NSW, Australia, selected from 68 BVR obs 2016 Jun. 11.63091-11.78534);
11.63216, 13.2949 B +/-0.0130 (Starr, as above);
11.63332, 12.3166 V +/-0.0096 (Starr, as above);
11.67197, 12.2 (PAW, A. Plummer, Linden, NSW, Australia);
11.70072, 11.3373 CV +/-0.0122 (Starr, as above);
11.70197, 13.5749 B +/-0.0059 (Starr, as above);
11.70312, 12.3926 V +/-0.0025 (Starr, as above);
11.78296, 11.2928 CV +/-0.0083 (Starr, as above);
11.78421, 13.5515 B +/-0.0072 (Starr, as above);
11.78534, 12.3602 V +/-0.0028 (Starr, as above);
11.99389, 12.037 V +/-0.008 (NRNA, R. Nogues Naves, Cabrils, Spain);
12.16295, 12.380 V +/-0.009 (Hambsch);
12.18378, 12.348 V +/-0.008 (Hambsch);
12.19627, 12.362 V +/-0.008 (Hambsch);
12.42710, 9.16 I +/-0.03 (OCN, S. O'Connor, St. George, Bermuda);
12.42800, 10.61 R +/-0.02 (O'Connor);
12.42880, 12.22 V +/-0.02 (O'Connor);
12.42990, 13.65 B +/-0.03 (O'Connor);
12.47258, 12.125 V +/-0.004 (NLX, P. Nelson, Ellinbank, VIC, Australia, selected from 266 V obs Jun. 12.47258-12.78428 UT);
12.57032, 12.173 V +/-0.004 (Nelson, as above);
12.67065, 12.197 V +/-0.006 (Nelson, as above);
12.77050, 12.251 V +/-0.008 (Nelson, as above);
12.78428, 12.351 V +/-0.009 (Nelson, as above);
13.19722, <12.6 (SLH, L. Shotter, Uniontown, PA);
13.43300, 13.92 B +/-0.02 (O'Connor);
13.43510, 12.60 V +/-0.01 (O'Connor);

Submit observations: Please submit observations to the AAVSO International Database using the name NOVA SCO 2016. Be sure to include spaces in name as shown.

Notes:
done a. Announced in IAU Central Bureau for Astronomical Telegrams Central Bureau Electronic Telegram 4285 (Daniel W. E. Green, ed.). Designated PNV J17381927-3725077 when when posted to the IAU CBAT Transient Object Confirmation Page (TOCP). Most of the information in this Alert Notice is taken from IAU CBET 4285.

b. P. Schmeer (Bischmisheim, Germany) reports a star of red magnitude 17.1-17.4 in the USNO-B1.0 catalogue with position end figures 19.26s, 07.7". Schmeer also reports a potentially better progenitor candidate on the Digitized Sky Survey infrared image just southwest of the USNO-B1.0 star.

c. Position end figures (from CBET 4285):
 - T. Kojima (Tsumagoi, Gunma-ken, Japan, pre-discovery image on three frames), 2016 Jun. 9.596 UT, 18.8s, 10"
 - H. Nishimura (discovery), 2016 June 10.629 UT, 19.27s, 07.7"
 - K. Itagaki (Yamagata, Japan), 2016 Jun. 11.506 UT, 19.22s, 07.8"
 - T. Noguchi (Katori, Chiba-ken, Japan), 2016 Jun. 11.513 UT, 19.27s, 09.1"

d. Images posted (from CBET 4285):
 - S. Kiyota (Kamagaya, Japan), 2016 Jun. 11.255 UT:
http://meineko.sakura.ne.jp/ccd/PNV_J17381927-3725077.jpg
- T. Noguchi (Katori, Chiba-ken, Japan), 2016 Jun. 11.513 UT:
http://park8.wakwak.com/~ngc/images/PNVinSco_20160611.jpg

Congratulations to Hideo Nishimura on his latest discovery!

This AAVSO Alert Notice was compiled by Elizabeth O. Waagen.



It’s all about the  standstills, those episodes where the star gets stuck at a mid-point between maximum and minimum. If it doesn’t exhibit standstills it isn’t a Z Cam star.






AM Her stars in need of further investigation








Data from Catalina Real Time Survey 
Drake et al. 2009, ApJ, 696, 87

Northern CVs brighter than 17th magnitude here.

Southern CV's brighter than 17th magnitude here.



ACTIVITY AT A GLANCE

New outbursts and unusual activity reported in the last 72 hours

Last updated 15:46 UT June 24, 2016

YYYYMMDD

20160623
TU Crt
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# indicates a noteworthy or unusual outburst
 
'Activity At A Glance' is gleaned from observations reported to AAVSO MyNewsFlash, BAAVSS-Alert, CVnet-Outburst, VSObs-share and VSNET-outburst. We sincerely thank all the observers who contribute timely observations and reports of activity to these email lists.

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