2019A&A...624A..53M


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.02CEST14:08:22

2019A&A...624A..53M - Astronomy and Astrophysics, volume 624A, 53-53 (2019/4-1)

The two tails of PSR J2055+2539 as seen by Chandra: Analysis of the nebular morphology and pulsar proper motion.

MARELLI M., TIENGO A., DE LUCA A., MIGNANI R.P., SALVETTI D., SAZ PARKINSON P.M. and LISINI G.

Abstract (from CDS):

We analyzed two Chandra observations of PSR J2055+2539 for a total integration time of ∼130ks to measure the proper motion and study the two elongated nebular features of this source. We did not detect the proper motion, setting an upper limit of 240mas/yr (3σ level), which translates into an upper limit on the transverse velocity of ∼700km/s, for an assumed distance of 600pc. A deep Hα observation did not reveal the bow shock associated with a classical pulsar wind nebula, thus precluding an indirect measurement of the proper motion direction. We determined the main axes of the two nebulae, which are separated by an angle of 160.8°±0.7°, using a new approach based on the rolling Hough transformation (RHT). We analyzed the shape of the first 8' (out of the 12' seen by XMM-Newton) of the brighter, extremely collimated nebula. Based on a combination of our results from a standard analysis and a nebular modeling obtained from the RHT, we find that the brightest nebula is curved on an arcmin scale and has a thickness ranging from ∼9'' to ∼31'' and a possible (single or multiple) helicoidal pattern. We could not constrain the shape of the fainter nebula. We discuss our results in the context of other known similar features and place particular emphasis on the Lighthouse nebula associated with PSR J1101-6101. We speculate that a peculiar geometry of the powering pulsar may play an important role in the formation of such features.

Abstract Copyright: © ESO 2019

Journal keyword(s): techniques: image processing - methods: data analysis - stars: neutron - X-rays: general - stars: winds, outflows - stars: individual: PSR J2055+2539

Simbad objects: 8

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Number of rows : 8

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 PSR J0357+32 Psr 03 57 52.161 +32 05 23.63           ~ 75 0
2 PSR B0355+54 Psr 03 58 53.7165 +54 13 13.727           ~ 388 1
3 PSR B0656+14 Psr 06 59 48.183 +14 14 21.54   24.85 24.90     ~ 758 1
4 IGR J11014-6103 gam 11 01 45.05 -61 01 40.3           ~ 36 0
5 NGC 3561 LIN 11 11 13.2 +28 41 47   14.7       ~ 191 2
6 PSR J1509-5850 Psr 15 09 27.153 -58 50 56.05           ~ 94 0
7 PSR J2055+25 Psr 20 55 48.948 +25 39 58.93           ~ 38 0
8 PSR B2223+65 Psr 22 25 52.36 +65 35 33.8           ~ 286 0

    Equat.    Gal    SGal    Ecl

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2020.07.02-14:08:22

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