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Query : 2013MNRAS.431L..33N |
2013MNRAS.431L..33N - Mon. Not. R. Astron. Soc., 431, L33-L37 (2013/May-1)
The dusty aftermath of the V1309 Sco binary merger.
NICHOLLS C.P., MELIS C., SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., KUBIAK M., PIETRZYNSKI G., POLESKI R., ULACZYK K., WYRZYKOWSKI L., KOZLOWSKI S. and PIETRUKOWICZ P.
Abstract (from CDS):
Model fits to the solid-state absorption feature constrain the constituent species and column density of the dust around V1309 Sco. We find that the absorption feature can be reproduced by large (3µm) amorphous pyroxene grains at a temperature of 800 K. This grain size, if confirmed with longer wavelength spectroscopy and modelling, would be suggestive of dust processing in the circumstellar environment. The data in hand do not allow us to discriminate between disc or shell configurations for the dusty material.
Abstract Copyright: © 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2013)
Journal keyword(s): binaries: close - circumstellar matter - stars: individual: V1309 Sco
Simbad objects: 6
Number of rows : 6 |
N | Identifier | Otype |
ICRS (J2000) RA |
ICRS (J2000) DEC |
Mag U | Mag B | Mag V | Mag R | Mag I | Sp type |
#ref
1850 - 2024 |
#notes |
---|---|---|---|---|---|---|---|---|---|---|---|---|
1 | NAME Magellanic Clouds | GrG | 03 00 | -71.0 | ~ | 7067 | 0 | |||||
2 | V* V838 Mon | No* | 07 04 04.8221494992 | -03 50 50.648894412 | 15.181 | 14.51 | M10+B3V | 427 | 0 | |||
3 | V* FK Com | PM* | 13 30 46.7996390256 | +24 13 57.781233768 | 9.04 | 8.245 | 7.204 | G4III | 372 | 1 | ||
4 | NAME Galactic Center | reg | 17 45 39.60213 | -29 00 22.0000 | ~ | 14420 | 0 | |||||
5 | V* V1309 Sco | No* | 17 57 32.9368332984 | -30 43 09.965039880 | 16.9 | 14.8 | ~ | 261 | 0 | |||
6 | V* V4332 Sgr | CV* | 18 50 36.6958376520 | -21 23 28.925017944 | 14.37 | K8/M0e | 174 | 0 |
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