2014A&A...569L...4C


C.D.S. - SIMBAD4 rel 1.7 - 2021.02.26CET23:40:18

2014A&A...569L...4C - Astronomy and Astrophysics, volume 569, L4-4 (2014/9-1)

The RCB star V854 Centauri is surrounded by a hot dusty shell.

CHESNEAU O., MILLOUR F., DE MARCO O., BRIGHT S.N., SPANG A., LAGADEC E., MEKARNIA D. and DE WIT W.J.

Abstract (from CDS):

The hydrogen-deficient supergiants known as R Coronae Borealis (RCB) stars might be the result of a double-degenerate merger of two white dwarfs (WDs), or a final helium shell flash in a planetary nebula central star. In this context, any information on the geometry of their circumstellar environment and, in particular, the potential detection of elongated structures, is of great importance. We obtained near-IR observations of V854 Cen with the AMBER recombiner located at the Very Large Telescope Interferometer (VLTI) array with the compact array (B≤35m) in 2013 and the long array (B≤140m) in 2014. At each time, V854 Cen was at maximum light. The H- and K-band continua were investigated by means of spectrally dependant geometric models. These data were supplemented with mid-IR VISIR/VLT images. A dusty slightly elongated overdensity is discovered both in the H- and K-band images. With the compact array, the central star is unresolved (Θ≤2.5mas), but a flattened dusty environment of 8x11 mas is discovered whose flux increases from about ∼20% in the H band to reach about ∼50% at 2.3µm, which indicates hot (T∼1500K) dust in the close vicinity of the star. The major axis is oriented at a position angle (PA) of 126±29°. Adding the long-array configuration dataset provides tighter constraints on the star diameter (Θ≤1.0mas), a slight increase of the overdensity to 12x15mas and a consistent PA of 133±49°. The closure phases, sensitive to asymmetries, are null and compatible with a centro-symmetric, unperturbed environment excluding point sources at the level of 3% of the total flux in 2013 and 2014. The VISIR images exhibit a flattened aspect ratio at the 15-20% level at larger distances (∼1") with a position angle of 92±19°, marginally consistent with the interferometric observations. This is the first time that a moderately elongated structure has been observed around an RCB star. These observations confirm the numerous suggestions for a bipolar structure proposed for this star in the literature, which were mainly based on polarimetric and spectroscopic observations.

Abstract Copyright:

Journal keyword(s): techniques: high angular resolution - stars: individual: V854 Cen - circumstellar matter - stars: mass-loss

Simbad objects: 9

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Number of rows : 9

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 V* V838 Mon CV* 07 04 04.8222936785 -03 50 50.637499515   15.5   15.18 14.51 M10+B3V 378 0
2 HD 124433 PM* 14 14 42.6612475577 -41 50 14.972424053   6.535 5.613     G8III 15 0
3 V* V853 Cen dS* 14 29 58.3584825657 -56 07 52.462145481   7.189 6.965     A6V 46 0
4 HD 127214 * 14 31 11.2848030961 -40 23 11.127155307   7.73 6.75     G8/K0III 7 0
5 V* V854 Cen RC* 14 34 49.4088471574 -39 33 19.276531885   7.13 11.69     Ce 201 0
6 V* V4334 Sgr NL* 17 52 32.69 -17 41 08.0   12.01       F2Ia 338 0
7 V* V1309 Sco CV* 17 57 32.9383021931 -30 43 09.967391199   16.9   14.8   ~ 187 0
8 V* V4332 Sgr CV* 18 50 36.6959119600 -21 23 28.927014456         14.37 K8/M0e 148 0
9 V* RY Sgr RC* 19 16 32.7669543079 -33 31 20.337025534 6.20 6.27 6.25     Cpec 356 0

    Equat.    Gal    SGal    Ecl

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2021.02.26-23:40:18

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