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| Query : 2014A&A...565A..82N |
2014A&A...565A..82N - Astronomy and Astrophysics, volume 565A82-82 (2014/5-1)
Symbiotic stars in X-rays. II. Faint sources detected with XMM-Newton and Chandra.
NUNEZ N.E., LUNA G.J.M., PILLITTERI I. and MUKAI K.
Abstract (from CDS):
We report the detection from four symbiotic stars that were not known to be X-ray sources. These four object show a β-type X-ray spectrum, that is, their spectra can be modeled with an absorbed optically thin thermal emission with temperatures of a few million degrees. Photometric series obtained with the Optical Monitor on board XMM-Newton from V2416 Sgr and NSV 25735 support the proposed scenario where the X-ray emission is produced in a shock-heated region inside the symbiotic nebulae.
Abstract Copyright: ∼
Journal keyword(s): binaries: symbiotic - X-rays: binaries
Simbad objects: 10
| Number of rows : 10 |
| 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 | * omi Cet | Mi* | 02 19 20.79210 | -02 58 39.4956 | 7.63 | 6.53 | 5.03 | M5-9IIIe+DA | 1586 | 0 | ||
| 2 | EM* MWC 560 | Sy* | 07 25 51.2842107720 | -07 44 08.084175396 | 10.01 | 9.70 | 10.60 | M4ep+Beq | 223 | 0 | ||
| 3 | EM* AS 201 | PN | 08 31 42.8828281680 | -27 45 31.543524864 | 13 | 11.80 | F9III | 96 | 0 | |||
| 4 | HD 311884 | WR* | 12 43 50.9991209208 | -63 05 14.812489320 | 11.45 | 11.64 | 10.81 | 10.59 | WN6+O5V | 175 | 0 | |
| 5 | WRAY 16-119 | LP? | 12 45 47.0072068008 | -63 00 35.643508344 | 16.60 | 16.61 | M7.5 | 44 | 2 | |||
| 6 | WRAY 16-147 | Sy* | 14 11 52.0604355768 | -51 26 24.187122024 | 14.20 | ~ | 240 | 1 | ||||
| 7 | HD 330036 | PN | 15 51 15.9290064932 | -48 44 58.559111355 | 11.759 | 10.892 | 10.921 | F5III-IVe | 164 | 0 | ||
| 8 | Ve 3-61 | Sy* | 17 57 16.0073137848 | -21 41 29.107661424 | M7/9e | 71 | 2 | |||||
| 9 | EM* StHA 190 | Sy* | 21 41 44.8876442736 | +02 43 54.414342804 | 11.13 | 10.22 | G5e | 55 | 0 | |||
| 10 | V* R Aqr | Sy* | 23 43 49.4634303216 | -15 17 04.176349872 | 8.823 | 7.683 | 9.37 | M6.5-8.5e | 823 | 0 |
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