A tale of two populations: rotating radio transients and x-ray dim isolated neutron stars - INSPIRE

DataBETA

A tale of two populations: rotating radio transients and x-ray dim isolated neutron stars

Sergei B. Popov
(
- Sternberg Astron. Inst.
)
,
R. Turolla
(
- Padua U.
)
,
A. Possenti
(
- Cagliari Observ.
)

Mar, 2006

5 pages

Published in:

Mon.Not.Roy.Astron.Soc. 369 (2006) L23-L26

e-Print:

astro-ph/0603258 [astro-ph]

DOI:

10.1111/j.1745-3933.2006.00166.x

View in:

ADS Abstract Service

reference search50 citations

Citations per year

Abstract: (arXiv)

We highlight similarities between recently discovered Rotating Radio Transients and X-ray Dim Isolated Neutron Stars. In particular, it is shown that X-ray Dim Isolated Neutron Stars have a birthrate comparable to that of Rotating Radio Transients. On the contrary, magnetars have too low a formation rate to account for the bulk of the radio transient population. The consequences of the recent detection of a thermal X-ray source associated with one of the Rotating Radio Transients on the proposed scenarios for these sources are also discussed.

stars: evolution
stars: neutron
pulsars: general

References(41)

Figures(0)

Candidate isolated neutron stars and other optically blank x-ray fields identified from the rosat all-sky and sloan digital sky surveys

et al.

- Astron.J. 131 (2006) 1740-1749
•
e-Print:
- astro-ph/0511659
•
DOI:
- 10.1086/500049

- Astrophys.J. 544 1245

Statistics of extinct radio pulsars

V.S. Beskin
(
- Lebedev Inst.
)
,
Svetlana A. Eliseeva
(
- Moscow, MIPT
)

- Astron.Lett. 31 (2005) 263-270
•
e-Print:
- astro-ph/0508409
•
DOI:
- 10.1134/1.1896070

Statistics of neutron stars at the stage of supersonic propeller

V.S. Beskin
(
- Lebedev Inst.
)
,
Svetlana A. Eliseeva
(
- Moscow, MIPT
)

- Astron.Lett. 31 (2005) 579-585
•
e-Print:
- astro-ph/0508442
•
DOI:
- 10.1134/1.2039968

Cooling of neutron stars: Hadronic model

David Blaschke
(
- Rostock U. and
- Dubna, JINR
)
,
H. Grigorian
(
- Rostock U. and
- Yerevan State U.
)
,
D.N. Voskresensky
(
- Darmstadt, GSI and
- Moscow Phys. Eng. Inst.
)

- Astron.Astrophys. 424 (2004) 979-992
•
e-Print:
- astro-ph/0403170
•
DOI:
- 10.1051/0004-6361:20040404

The implications of radio-quiet neutron stars

- Mon.Not.Roy.Astron.Soc. 305 (1999) 671
•
e-Print:
- astro-ph/9803176
•
DOI:
- 10.1046/j.1365-8711.1999.02490.x

Blank field sources in the ROSAT HRI Brera Multiscale Wavelet Catalog

M. Chieregato
(
- Insubria U., Como and
- Zurich U.
)
,
S. Campana
(
- Brera Observ.
)
,
A. Treves
(
- Insubria U., Como
)
,
A. Moretti
(
- Brera Observ.
)
,
R.P. Mignani
(
- European Southern Observ.
)

et al.

- Astron.Astrophys. 444 (2005) 69
•
e-Print:
- astro-ph/0505292
•
DOI:
- 10.1051/0004-6361:20041726

Radioactive Al-26 and massive stars in the galaxy

et al.

- Nature 439 (2006) 45-47
•
e-Print:
- astro-ph/0601015
•
DOI:
- 10.1038/nature04364

Birth and evolution of isolated radio pulsars

- Astrophys.J. 643 (2006) 332-355
•
e-Print:
- astro-ph/0512585
•
DOI:
- 10.1086/501516

- Astron.Astrophys. 287 L21

Gamma-ray sources as relics of recent supernovae in the nearby gould belt

I.A. Grenier

- Astron.Astrophys. 364 (2000) L93
•
e-Print:
- astro-ph/0011298

AXPs and X-ray-dim isolated neutron stars: recent XMM-Newton and Chandra results

Frank Haberl
(
- Garching, Max Planck Inst., MPE
)

- Adv.Space Res. 33 (2004) 4, 638-644
•
e-Print:
- astro-ph/0302540
•
DOI:
- 10.1016/j.asr.2003.07.022

- Mon.Not.Roy.Astron.Soc. 340 L43

The parallax and proper motion of rx j1856.5-3754 revisited

- Astrophys.J. 571 (2002) 447
•
e-Print:
- astro-ph/0111174
•
DOI:
- 10.1086/339879

A Coherent timing solution for the nearby isolated neutron star RX J0720.4-3125

- Astrophys.J.Lett. 628 (2005) L45-L48
•
e-Print:
- astro-ph/0506419
•
DOI:
- 10.1086/432536

A coherent timing solution for the nearby isolated neutron star rx j1308.6+2127/rbs 1223

- Astrophys.J.Lett. 635 (2005) L65-L68
•
e-Print:
- astro-ph/0511084
•
DOI:
- 10.1086/499241

Galactic structure from the Spacelab infrared telescope. 2. Luminosity models of the Milky Way

- Astrophys.J. 378 (1991) 131-138
•
DOI:
- 10.1086/170413

An X-ray pulsar with a superstrong magnetic field in the soft gamma-ray repeater SGR 1806-20.

et al.

- Nature 393 (1998) 235-237
•
DOI:
- 10.1038/30410

- Mon.Not.Roy.Astron.Soc. 362 L8

A braking index for the young pulsar at the center of the supernova remnant kes 75

- Astrophys.J. 647 (2006) 1286
•
e-Print:
- astro-ph/0601530
•
DOI:
- 10.1086/505570

- Astron.Rep. 49 242

Transient radio bursts from rotating neutron stars

et al.

- Nature 439 (2006) 817
•
e-Print:
- astro-ph/0511587
•
DOI:
- 10.1038/nature04440

On the number of accreting and cooling isolated neutron stars detectable with the rosat all-sky survey

- Astron.Astrophys. 343 (1999) 151
•
e-Print:
- astro-ph/9812455

Minimal cooling of neutron stars: A New paradigm

Dany Page
(
- UNAM, Inst. Astron.
)
,
James M. Lattimer
(
- SUNY, Stony Brook
)
,
Madappa Prakash
(
- SUNY, Stony Brook
)
,
Andrew W. Steiner
(
- Minnesota U.
)

- Astrophys.J.Suppl. 155 (2004) 623-650
•
e-Print:
- astro-ph/0403657
•
DOI:
- 10.1086/424844

The Neutron Stars Census

et al.

- Astrophys.J. 530 (2000) 896
•
e-Print:
- astro-ph/9910114
•
DOI:
- 10.1086/308408

1-25 of 41
1
2
25 / page