2019MNRAS.484.5791B


Query : 2019MNRAS.484.5791B

2019MNRAS.484.5791B - Mon. Not. R. Astron. Soc., 484, 5791-5801 (2019/April-3)

The High Time Resolution Universe Pulsar Survey - XV. Completion of the intermediate-latitude survey with the discovery and timing of 25 further pulsars.

BURGAY M., STAPPERS B., BAILES M., BARR E.D., BATES S., BHAT N.D.R., BURKE-SPOLAOR S., CAMERON A.D., CHAMPION D.J., EATOUGH R.P., FLYNN C.M.L., JAMESON A., JOHNSTON S., KEITH M.J., KEANE E.F., KRAMER M., LEVIN L., NG C., PETROFF E., POSSENTI A., VAN STRATEN W., TIBURZI C., BONDONNEAU L. and LYNE A.G.

Abstract (from CDS):

We report on the latest six pulsars discovered through our standard pipeline in the intermediate-latitude region (|b| < 15°) of the Parkes High Time Resolution Universe Survey (HTRU). We also present timing solutions for the new discoveries and for 19 further pulsars for which only discovery parameters were previously published. Highlights of the presented sample include the isolated millisecond pulsar J1826-2415, the long-period binary pulsar J1837-0822 in a mildly eccentric 98-d orbit with a >0.27 M☉ companion, and the nulling pulsar J1638-4233, detected only 10 per cent of the time. Other interesting objects are PSR J1757-1500, exhibiting sporadic mode changes, and PSR J1635-2616 showing one glitch over 6 yr. The new discoveries bring the total count of HTRU intermediate-latitude pulsars to 113, 25 per cent of which are recycled pulsars. This is the highest ratio of recycled over ordinary pulsars discoveries of all recent pulsar surveys in this region of the sky. Among HTRU recycled pulsars, four are isolated objects. Comparing the characteristics of Galactic fully recycled isolated MSPs with those of eclipsing binaries ('spiders'), from which the former are believed to have formed, we highlight a discrepancy in their spatial distribution. This may reflect a difference in the natal kick, hence, possibly, a different formation path. On the other hand, however, isolated fully recycled MSPs spin periods are, on average, longer than those of spiders, in line with what one would expect, from simple magnetic-dipole spin-down, if the former were indeed evolved from the latter.

Abstract Copyright: © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): pulsars: individual: (J1635-2616, J1638-4233, J1757-1500, J1826-2415, J1837-0822)

Simbad objects: 41

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Number of rows : 41
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 NAME Per Arm PoG 03 30 +45.0           ~ 1672 0
2 PSR B0736-40 Psr 07 38 32.2620 -40 42 39.420           ~ 212 0
3 PSR J0836-4233 Psr 08 36 05.85 -42 33 24.9           ~ 4 0
4 PSR J1105-4357 Psr 11 05 24.84 -43 53 05.0           ~ 4 0
5 PSR J1119-6127 Psr 11 19 14.30 -61 27 49.5           ~ 439 1
6 PSR J1132-4700 Psr 11 32 14.52 -47 00 36.5           ~ 5 0
7 PSR J1141-6545 Psr 11 41 07.00060 -65 45 19.0500     25.08 24.38   ~ 207 1
8 PSR J1518-3952 Psr 15 18 56.968 -39 52 30.30           ~ 4 0
9 PSR J1530-6343 Psr 15 30 47.608 -63 43 13.60           ~ 5 0
10 PSR J1551-6214 Psr 15 51 36.788 -62 14 23.37           ~ 5 0
11 PSR J1614-3846 Psr 16 14 42.52 -38 46 35.0           ~ 2 0
12 PSR J1629-3825 Psr 16 29 14.618 -38 25 29.30           ~ 4 0
13 PSR J1636-2614 Psr 16 36 11.506 -26 14 47.00           ~ 7 0
14 PSR J1638-4233 Psr 16 38 24.71 -42 33 55.0           ~ 2 0
15 M 13 GlC 16 41 41.634 +36 27 40.75     5.8     ~ 2291 0
16 PSR J1704-5236 Psr 17 04 40.569 -52 36 57.40           ~ 6 0
17 PSR J1719-14 Psr 17 19 10.076221 -14 38 01.00200           ~ 92 2
18 PSR J1719-2330 Psr 17 19 36.1 -23 30 14           ~ 2 0
19 PSR B1737-30.8 Psr 17 40 50.031 -30 52 04.10           ~ 55 1
20 PSR J1748-2446ad Psr 17 48 04.9 -24 46 04           ~ 141 1
21 PSR J1749-5417 Psr 17 49 47.06 -54 17 30.7           ~ 3 0
22 PSR J1757-1500 Psr 17 57 12.752 -15 00 28.50           ~ 3 0
23 PSR J1802-0523 Psr 18 02 12.14 -05 23 29.0           ~ 2 0
24 PSR J1804-2858 Psr 18 04 19.0 -28 58 31           ~ 9 0
25 PSR J1817-1938 Psr 18 17 06.82 -19 38 36.0           ~ 5 0
26 PSR J1818-0151 Psr 18 18 25.77 -01 51 54.0           ~ 5 0
27 PSR J1822-0848 Psr 18 22 51.86 -08 48 59.0           ~ 22 0
28 PSR J1824-0132 Psr 18 24 55.575 -01 32 24.00           ~ 8 0
29 PSR J1826-2415 Psr 18 26 36.0260 -24 15 54.500           ~ 2 0
30 PSR J1835-0847 Psr 18 35 45.72 -08 47 20.0           ~ 2 0
31 PSR J1837-0822 Psr 18 37 39.654 -08 22 12.40           ~ 4 0
32 PSR J1840-0445 Psr 18 40 45.5 -04 45 08           ~ 2 0
33 PSR J1900-0933 Psr 19 00 31.19 -09 33 48.1           ~ 5 0
34 PSR J1902-1036 Psr 19 02 42.399 -10 36 13.00           ~ 4 0
35 PSR J1904-1629 Psr 19 04 51.37 -16 29 19.0           ~ 1 0
36 PSR J1910+0517 Psr 19 10 37.907 +05 17 56.00           ~ 15 0
37 PSR J1920-0950 Psr 19 20 55.93 -09 50 01.0           ~ 3 0
38 PSR J1929+1357 Psr 19 29 10.62 +13 57 35.9           ~ 19 0
39 PSR J1932+1500 Psr 19 32 46.307 +15 00 22.20           ~ 7 0
40 PSR J1959+2048 Psr 19 59 36.7643141520 +20 48 14.896407996   21.08 20.16 19.53 18.79 G: 854 3
41 [MT91] 213 Psr 20 32 13.1247390384 +41 27 24.346666440 13.12 13.08 11.266     B0Vp 334 0

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