2017ApJ...836..135R

Query : 2017ApJ...836..135R

2017ApJ...836..135R - Astrophys. J., 836, 135-135 (2017/February-2)

Inferring the composition of super-Jupiter mass companions of pulsars with radio line spectroscopy.

RAY A. and LOEB A.

Abstract (from CDS):

We propose using radio line spectroscopy to detect molecular absorption lines (such as OH at 1.6-1.7 GHz) before and after the total eclipse of black widow and other short orbital period binary pulsars with low-mass companions. The companion in such a binary may be ablated away by energetic particles and high-energy radiation produced by the pulsar wind. The observations will probe the eclipsing wind being ablated by the pulsar and constrain the nature of the companion and its surroundings. Maser emission from the interstellar medium stimulated by a pulsar beam might also be detected from the intrabinary medium. The short temporal resolution allowed by the millisecond pulsars can probe this medium with the high angular resolution of the pulsar beam.

Abstract Copyright: © 2017. The American Astronomical Society. All rights reserved.

Journal keyword(s): binaries: eclipsing - interplanetary medium - ISM: molecules - masers - pulsars: general - radio lines: planetary systems - shock waves - shock waves

Simbad objects: 25

goto Full paper

goto View the references in ADS

Number of rows : 25
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 PSR J0751+1807 Psr 07 51 09.1539 +18 07 38.335           ~ 316 1
2 PSR J1012+5307 Psr 10 12 33.4345449600 +53 07 02.548542576     19.5     DA 419 1
3 PSR J1023+0038 Psr 10 23 47.6841824712 +00 38 41.005893516     17.31     GV 470 0
4 XSS J12270-4859 Psr 12 27 58.7476831464 -48 53 42.824592960           ~ 321 0
5 PSR B1257+12 Psr 13 00 03.1075 +12 40 55.155           ~ 546 1
6 CPD-63 2495 HXB 13 02 47.6544015048 -63 50 08.626970292 10.34 10.72 9.98 10.03   O9.5Ve 852 0
7 PSR J1311-3430 Psr 13 11 45.7292612136 -34 30 30.294149760   21.0   18.8   ~ 181 1
8 PSR B1620-26 Psr 16 23 38.2218 -26 31 53.769     21.30     ~ 318 2
9 PSR B1641-45 Psr 16 44 49.28482 -45 59 09.6360     12.60     ~ 217 0
10 PSR J1719-14 Psr 17 19 10.076221 -14 38 01.00200           ~ 92 2
11 PSR B1718-35 Psr 17 21 32.76 -35 32 48.3           ~ 86 0
12 PSR J1723-2837 Psr 17 23 23.1937506912 -28 37 57.210408048   16.81 15.77 15.71   ~ 105 0
13 PSR B1744-24A Psr 17 48 02.249 -24 46 37.65           ~ 235 0
14 PSR J1807-2459A Psr 18 07 20.36 -24 59 52.6           ~ 30 0
15 NGC 6544 GlC 18 07 20.58 -24 59 50.4   11.36 9.90     ~ 332 0
16 IGR J18245-2452 LXB 18 24 32.50 -24 52 07.8           ~ 253 0
17 M 28 GlC 18 24 32.89 -24 52 11.4           ~ 821 0
18 W 43 SFR 18 47 32 -01 56.5           ~ 604 0
19 PSR B1849+00 Psr 18 52 27.42 +00 32 02.0           ~ 76 0
20 PSR B1929+10 Psr 19 32 14.0570 +10 59 33.380           ~ 801 0
21 PSR B1937+21.4 Psr 19 39 38.560096 +21 34 59.13552           ~ 1142 0
22 PSR J1959+2048 Psr 19 59 36.7643141520 +20 48 14.896407996   21.08 20.16 19.53 18.79 G: 854 3
23 V* LY Aqr Psr 20 51 07.52058 -08 27 37.6100           ~ 236 2
24 PSR J2241-5236 Psr 22 41 42.03161 -52 36 36.2492           ~ 143 1
25 PSR J2339-0533 Psr 23 39 38.7412778376 -05 33 05.108592528     18.48     ~ 149 0

To bookmark this query, right click on this link: simbad:objects in 2017ApJ...836..135R and select 'bookmark this link' or equivalent in the popup menu