Sat, 02/24/2018 - 20:18
SASSN-18ds (N/UG)
"ASAS-SN Discovery of a Possible Galactic Nova ASASSN-18ds":
http://www.astronomerstelegram.org/?read=11348
RA 17:03:47.51, DEC -38:16:57.14 (J2000.0)
ASASSN-18ds 20180222.32 <177V ASN
ASASSN-18ds 20180224.36 143V ASN
VVV J170347.56-381658.24 = 2MASS J17034754-3816581 is 1" away.
Spectroscopy and time-resolved photometry are urgently required.
Clear skies,
Patrick
Meanwhile ASASSN-18ds reached 13,2V brightness:
https://asas-sn.osu.edu/light_curves/70597162-4120-4aee-be3f-b17e245eaa…
Robert
"The spectrum is dominated by the strong emission blend of Halpha and [NII]. In addition to the Balmer lines, strong FeII emission lines are present, blended with their respective blue-shifted absorption lines. We interpret the spectrum as that of an FeII-class nova during the pre-maximum phase.
Unfortunately, the object is slightly saturated on the R acquisition image. Comparing with the brightest star in the field, USNO 0450.26357218, which is not saturated, we find that the nova is brighter than R=12.4mag during our observation. This confirms that it is still on the rise to maximum."
http://www.astronomerstelegram.org/?read=11360
If I'm right this is the 6th galactic nova in 2018 and the 3rd in Sco.