X-Işınlarında Anlatılan Bir Kilonova’nın Açığa Çıkan Hikayesi

• <span class="glossaryLink" aria-describedby="tt" data-cmtooltip="
  NASA
  Established in 1958, the National Aeronautics and Space Administration (NASA) is an independent agency of the United States Federal Government that succeeded the National Advisory Committee for Aeronautics (NACA). It is responsible for the civilian space program, as well as aeronautics and aerospace research. It's vision is "To discover and expand knowledge for the benefit of humanity."

  ” data-gt-translate-attributes=”[{” attribute=””>NASA’s Chandra X-ray Observatory continues to study GW170817, a neutron star merger that produced gravitational waves.

• Many telescopes saw different kinds of light after the discovery in August 2017, but only Chandra is still making a detection.
• Early Chandra data revealed the presence of a narrow jet that has slowed down and expanded over time.
• The latest study presents X-ray evidence for a shock — similar to a sonic boom from an airplane — in the aftermath of the merger.

Bir sanatçının anlayışı, iki nötron yıldızı birleştiğinde meydana gelen güçlü bir olay olan “kilonova”nın sonrasını tasvir ediyor. NASA’nın Chandra X-ışını Gözlemevi, Lazer İnterferometri Yerçekimi Dalgası Gözlemevi tarafından yerçekimi dalgalarında ilk kez tespit edilmesinden kısa bir süre sonra GW170817 ile ilişkili kilonova hakkında veri toplamaktadır ([{” attribute=””>LIGO) and Virgo on August 17, 2017.

GW170817 was the first — and thus far the only — cosmic event where both gravitational waves and electromagnetic radiation, or light, were detected. This combination provides scientists with critical information about the physics of neutron star mergers and related phenomena, using observations at many different parts of the electromagnetic spectrum. Chandra is the only observatory still able to detect light from this extraordinary cosmic collision more than four years after the original event.

Astronomers think that after neutron stars merge, the debris generates visible and infrared light from the decay of radioactive elements like platinum and gold formed in the debris from the merger. This burst of light is called a kilonova. Indeed, visible light and infrared emission were detected from GW170817 several hours after the gravitational waves.

GW170817 X-ray. Credit: NASA/CXC/Northwestern Univ./A. Hajela et al.

Initially the neutron star merger likely produced a jet of high-energy particles that was not pointed directly at Earth, explaining an initial lack of X-rays seen by Chandra. The jet then slowed down and widened upon impact with surrounding gas and dust. These changes caused an increase in X-rays observed by Chandra followed by a decline in early 2018. However, since the end of 2020, the X-rays detected by Chandra have remained at a nearly constant level. The Chandra image from data taken in December 2020 and January 2021 shows X-ray emission from GW170817 and from the center of its host galaxy, NGC 4993.

A research team studying the Chandra data think this steadying of the X-ray emission comes from a shock — like a sonic boom from an airplane — as the merger debris responsible for the kilonova strikes gas around GW170817. Material heated by such a shock would glow steadily in X-rays giving a “kilonova afterglow”, like Chandra has observed. The artist’s illustration shows the merger debris responsible for the kilonova in blue surrounded by a shock depicted in orange and red.

There is also an alternative explanation suggesting that the X-rays come from material falling towards a black hole that formed after the neutron stars merged. This material is depicted by a small disk in the center of the illustration. To avoid a coincidence, it is likely that only one of the two options — the kilonova afterglow or matter falling onto a black hole — is a significant source of the detected X-rays.

The two blue glowing arcs of material above and below the kilonova show where material from the now-faded jet has struck surrounding material.

To distinguish between the two explanations astronomers will keep monitoring GW170817 in X-rays and radio waves. If it is a kilonova afterglow, the radio emission is expected to get brighter over time and be detected again in the next few months or years. If the explanation involves matter falling onto a newly-formed black hole, then the X-ray output should stay steady or decline rapidly and no radio emission will be detected over time.

Researchers recently announced a source was detected in new Chandra observations performed in December 2021. Analysis of that data is ongoing. No radio detection has yet been reported.

Bu araştırma hakkında daha fazla bilgi için bakınız:

Bu sonuçları açıklayan bir makale The Astrophysical Journal Letters’ın son sayısında yer almaktadır ve çevrimiçi olarak mevcuttur. https://scitechdaily.com/extraordinary-cosmic-collision-the-unfolding-story-of-a-kilonova-told-in-x-rays/. Yazarlar Aprajita Hajela’dır (kuzeybatı Üniversitesi), Rafella Marguitti (University of California at Berkeley), Joe Bright (Berkeley), Kate Alexander (Kuzeybatı), Brian Metzger (Kolombiya Üniversitesi), Vsevovold Nedora (University of Jena, Almanya), Adithan Kathirgamarju (Berkeley), Ben Margalit (Berkeley), David Radice (Penn State Üniversitesi), Cristiano Guidorzi (Ferrara Üniversitesi, İtalya), Edo Berger (Center for Astrophysics I Harvard & Smithsonian (CfA)), Andrew MacFadyen (New York Üniversitesi), Dimitrios Giannios (Purdue Üniversitesi), Ryan Chornock (Berkeley), Ian Heywood (Oxford Üniversitesiİngiltere), Lorenzo Sironi (Columbia), Ore Gottlieb (Tel Aviv Üniversitesi, İsrail), Deanne Coppjans (Kuzeybatı), Tanmoy Laskar (Bath Üniversitesi, Birleşik Krallık), Yvette Cendes (CfA), Rodolfo Barniol Duran (California Eyalet Üniversitesi, Sacramento), Tarraneh Eftekhari (CfA), Wen-fai Fong (Kuzeybatı), Austin McDowell (NYU), Matt Nicholl (Birmingham ÜniversitesiBirleşik Krallık), Zhengtong Xie (Southampton Üniversitesi, Birleşik Krallık), Jonathan Zrake (Clemson Üniversitesi), Sebastiano Bernuzzi (Jena Üniversitesi), Floor Broekgaarden (CfA), Charlie Kilpatrick (Kuzeybatı), Giacomo Terreran (Kuzeybatı), Ashley Villar ( Columbia), Peter Blanchard (Kuzeybatı), Sebastian Gomez (CfA), Griffin Hosseinzadeh (Arizona Üniversitesi), David Jacob Matthews (Berkeley) ve Jillian Rastinejad (Kuzeybatı).

NASA’nın Marshall Uzay Uçuş Merkezi, Chandra programını yönetiyor. Smithsonian Astrofizik Gözlemevi’nin Chandra X-ray Merkezi, Cambridge, Massachusetts’teki bilim operasyonlarını ve Burlington, Massachusetts’teki uçuş operasyonlarını kontrol ediyor.