2010A&A...518L.137V


Query : 2010A&A...518L.137V

2010A&A...518L.137V - Astronomy and Astrophysics, volume 518, L137-137 (2010/7-2)

Herschel images of NGC 6720: H2 formation on dust grains.

VAN HOOF P.A.M., VAN DE STEENE G.C., BARLOW M.J., EXTER K.M., SIBTHORPE B., UETA T., PERIS V., GROENEWEGEN M.A.T., BLOMMAERT J.A.D.L., COHEN M., DE MEESTER W., FERLAND G.J., GEAR W.K., GOMEZ H.L., HARGRAVE P.C., HUYGEN E., IVISON R.J., JEAN C., LEEKS S.J., LIM T.L., OLOFSSON G., POLEHAMPTON E.T., REGIBO S., ROYER P., SWINYARD B.M., VANDENBUSSCHE B., VAN WINCKEL H., WAELKENS C., WALKER H.J. and WESSON R.

Abstract (from CDS):

Herschel PACS and SPIRE images have been obtained of NGC 6720 (the Ring nebula). This is an evolved planetary nebula with a central star that is currently on the cooling track, due to which the outer parts of the nebula are recombining. From the PACS and SPIRE images we conclude that there is a striking resemblance between the dust distribution and the H2 emission, which appears to be observational evidence that H2 forms on grain surfaces. We have developed a photoionization model of the nebula with the Cloudy code which we used to determine the physical conditions of the dust and investigate possible formation scenarios for the H2. We conclude that the most plausible scenario is that the H2 resides in high density knots which were formed after the recombination of the gas started when the central star entered the cooling track. Hydrodynamical instabilities due to the unusually low temperature of the recombining gas are proposed as a mechanism for forming the knots. H2 formation in the knots is expected to be substantial after the central star underwent a strong drop in luminosity about one to two thousand years ago, and may still be ongoing at this moment, depending on the density of the knots and the properties of the grains in the knots.

Abstract Copyright:

Journal keyword(s): planetary nebulae: individual: NGC 6720 - circumstellar matter - dust, extinction - infrared: ISM - ISM: molecules

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 NAME Ophiuchus Molecular Cloud SFR 16 28 06 -24 32.5           ~ 3446 1
2 M 57 PN 18 53 35.0967659112 +33 01 44.883287544   15.405 15.769 15.901 16.062 DA(O?) 818 2
3 NGC 7293 PN 22 29 38.5454047152 -20 50 13.747242408 11.894 13.158 13.524 13.689 13.898 DAO.5 930 0

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2023.01.30-22:17:12

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