Team Taylor Jesus, Jason, Eric, Carl, Franz, Austin, Joey, Greg, and Jennifer.

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Presentation transcript:

Team Taylor Jesus, Jason, Eric, Carl, Franz, Austin, Joey, Greg, and Jennifer.

A known pulsar pulse profile has exact characteristics as the one below Pulsar distance from earth: light years Galactic latitude: -0.5 degrees Galactic longitude: 37.2 degrees Epn source (one below) is at.4 GHz Source on right is at 350 MHz Maximum DM: 1037

There is no way to fix or correct scattering.

Sources EPN ATNF pulsar catalog

Franz

For Galactic longitude 28.3 degrees and latitude degrees, and a dispersion measure of 36.1 cm - 3 pc, the estimated distance to your source is 1.5 kpc. The maximum DM predicted by the model for this direction is 86.5 cm -3 pc.

rDefined=true&c1_val=&c2_val=&c3_val=&c4_val=&sort_attr=jname&sort_order=asc&condition=&pulsar_names=&ephemeris=short&coords_unit=raj%2Fdecj&ra dius=3&coords_1=20%3A03%3A00&coords_2=- 13%3A44%3A00&style=Short+without+errors&no_value=*&fsize=3&x_axis=&x_scale=linear&y_axis=&y_scale=linear&state=query

Initial Observation DM: pc cm -3 Maximum DM for region: 39.5 pc cm -3 Reduced Χ 2:

Follow-up Observation P topo (ms) ≈8.806 (consistent with electrical interference)

White Dwarf Companion This pulsar is in orbit with a white dwarf. It is about 0.6 kpc or 1900 light-years away. As the pulsar moves away from Earth its pulse becomes delayed, but begins to arrive earlier as its orbit starts to bring it back towards Earth. The white dwarf in orbit with this pulsar is extremely tiny even for a white dwarf.

Black Widow Pulsar Credit: NASA/CXC/M.Weiss It is believed that extreme conditions on the pulsar generate high-energy particle winds that blast the surface of the white dwarf, slowly evaporating it. B. W. Stappers, et al., An x-ray nebula associated with the millisecond pulsar b Science 299 : 1372–1374 (2003).

Supernova