ScholarLens Back to search
1995•arXiv (Cornell University)Open access

A search for X-rays from five pulsars: PSR's 0740-28, 1737-30, 1822-09,\n 1915+13 and 1916+14

M. A. Alpar, O. H. Guseinov, Ü. Kızıloğlu, Ogelman, H.

Open full text 1 citations

Abstract

We report observations of PSR's 0740-28, 1737-30, 1822-09, 1915+13 and\n1916+14 with ROSAT. In the 0.1-2.1 keV range upper limits to luminosity are\nderived for power law and blackbody spectra, using a range of $N_{H}$\nestimates. The upper limit to the blackbody luminosity from PSR1822-09 turns\nout to be consistent with standard cooling curves. For the other pulsars the\nupper limits are not restrictive as they are much larger than the luminosities\npredicted by the models.\n

Open-access reader

About this research paper

What this paper is about

We report observations of PSR's 0740-28, 1737-30, 1822-09, 1915+13 and\n1916+14 with ROSAT. In the 0.1-2.1 keV range upper limits to luminosity are\nderived for power law and blackbody spectra, using a range of $N_{H}$\nestimates. The upper limit to the blackbody luminosity from PSR1822-09 turns\nout to be consistent with standard cooling curves. For the other pulsars the\nupper limits are not restrictive as they are much larger than the luminosities\npredicted by the models.\n

Why it matters

OpenAlex reports 1 citations for this work. Citation counts describe recorded attention and do not establish research quality.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Available abstract

We report observations of PSR's 0740-28, 1737-30, 1822-09, 1915+13 and\n1916+14 with ROSAT. In the 0.1-2.1 keV range upper limits to luminosity are\nderived for power law and blackbody spectra, using a range of $N_{H}$\nestimates. The upper limit to the blackbody luminosity from PSR1822-09 turns\nout to be consistent with standard cooling curves. For the other pulsars the\nupper limits are not restrictive as they are much larger than the luminosities\npredicted by the models.\n

Key concepts: Pulsar, Black-body radiation, ROSAT, Physics, Luminosity, Astrophysics, Limit (mathematics), Range (aeronautics)

Related papers

Related paper 1Related paper 2Related paper 3
Back to paper searchBrowse research topicsOriginal source
A search for X-rays from five pulsars: PSR's 0740-28, 1737-30, 1822-09,\n 1915+13 and 1916+14 — Research Paper | ScholarLens