<--- Back to Details
First PageDocument Content
Astronomy / Stellar evolution / Star types / Astrophysics / White dwarf / Planetary nebula / Binary star / Asymptotic giant branch / X-ray astronomy / Infrared excess / Stellar classification / Supernova
Date: 2015-06-01 09:58:04
Astronomy
Stellar evolution
Star types
Astrophysics
White dwarf
Planetary nebula
Binary star
Asymptotic giant branch
X-ray astronomy
Infrared excess
Stellar classification
Supernova

Add to Reading List

Source URL: www.astro.keele.ac.uk

Download Document from Source Website

File Size: 200,09 KB

Share Document on Facebook

Similar Documents

Seminar 1 – 1. Letnik, 2. Stopnja BINARY STAR SYSTEMS Avtor: Gašper Novak Mentor: Tomaž Zwitter Ljubljana, april 2018

DocID: 1v5PF - View Document

PREDICTING THE AFTERMATH OF THE NEUTRON STAR COLLISION THAT PRODUCED GW170817 The source of the gravitational-wave signal GW170817, very likely a binary neutron star merger, was also observed electromagnetically, providi

DocID: 1tL5A - View Document

SEARCHING FOR THE NEUTRON STAR OR BLACK HOLE RESULTING FROM GW170817 With the detection of a binary neutron star merger by the Advanced Laser Interferometer Gravitational Wave Observatory (LIGO) and Virgo, a natural ques

DocID: 1tKtW - View Document

GRAVITATIONAL WAVES AND GAMMA-RAYS FROM A BINARY NEUTRON STAR MERGER: GW170817 AND GRB 170817A The gravitational-wave signal GW170817 was detected on August 17, 2017 by the Advanced LIGO and Virgo observatories. This is

DocID: 1tJpU - View Document

MEASURING THE EXPANSION OF THE UNIVERSE WITH GRAVITATIONAL WAVES In August 2017 Advanced LIGO and Advanced Virgo detected gravitational waves from a binary neutron star merger for the very first time. This ground-breakin

DocID: 1tHe4 - View Document