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| Query : 2003IAUC.8158....2F |
2003IAUC.8158....2F - IAU Circ., 8158, 2 (2003/June-0)
No nova in NGC 6822.
FILIPPENKO A.V. and CHORNOCK R.
Abstract (from CDS):
Filippenko and Chornock report that inspection of CCD spectra (range 320-990 nm), obtained as above on June 29 UT, reveals that the apparent nova in NGC 6822 (cf. IAUC 8141) is actually a very late M-type star in that galaxy. Strong TiO bands are present, as is narrow H-alpha emission. Such stars are known to sometimes be highly variable, such as Mira variables.
Abstract Copyright: ∼
Journal keyword(s):
Simbad objects: 2
| Number of rows : 2 |
| N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2026 |
#notes |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | NGC 6822 | G | 19 44 56.199 | -14 47 51.29 | 18 | 8.1 | ~ | 1661 | 0 | |||
| 2 | [M98a] NGC 6822c-140 | Mi* | 19 45 04.080 | -14 45 46.96 | 20.14 | ~ | 8 | 0 |
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