GRB 150101B

{{use dmy dates|date=October 2018}}

{{Infobox astronomical event

| image = NASA-GRB150101B-Detection-January2015.jpg

| caption = Detection of GRB150101B

| type = ?? GRB, short-duration

| epoch = J2000

| redshift = ?? 0.093

| constellation = Virgo{{cite web |author=Staff |title=Finding the constellation which contains given sky coordinates |url=http://djm.cc/constellation.html |date= |work=DJM.cc |accessdate=17 October 2018 }}

| ra = {{RA|12|32|04.96}}

| dec = {{DEC|-10|56|00.7}}

| gal = 295.26103 +51.64971 [ 1800 1800 0 ]

| discovery = 1 January 2015
15:23 UT by the Burst Alert Telescope (BAT);
15:23:35 UT by the Gamma-ray Burst Monitor (GBM)

| distance = {{convert|1.7|e9ly|Gpc|lk=on}}
z=0.13437; 0.1341

| energy = ~1.3 {{e|49}} ergs

| names =

}}

GRB 150101B is a short gamma-ray burst (sGRB, or simply GRB) that was detected on 1 January 2015 at 15:23 UT by the Burst Alert Telescope (BAT) on board the Swift Observatory Satellite, and at 15:23:35 UT by the Gamma-ray Burst Monitor (GBM) on board the Fermi Gamma-ray Space Telescope.{{Cite journal |last1=Burns |first1=E. |last2=Veres |first2=P. |last3=Connaughton |first3=V. |last4=Racusin |first4=J. |last5=Briggs |first5=M. S. |last6=Christensen |first6=N. |last7=Goldstein |first7=A. |last8=Hamburg |first8=R. |last9=Kocevski |first9=D. |last10=McEnery |first10=J. |last11=Bissaldi |first11=E. |last12=Canton |first12=T. Dal |last13=Cleveland |first13=W. H. |last14=Gibby |first14=M. H. |last15=Hui |first15=C. M. |date=2018-08-17 |title=Fermi GBM Observations of GRB 150101B: A Second Nearby Event with a Short Hard Spike and a Soft Tail |journal=The Astrophysical Journal |volume=863 |issue=2 |pages=L34 |doi=10.3847/2041-8213/aad813 |s2cid=119489650 |issn=2041-8213|doi-access=free |arxiv=1807.02866 }} The GRB was determined to be {{convert|1.7|e9ly|Gpc|lk=on}} from Earth near the host galaxy 2MASX J12320498-1056010 {{cite web |author=Staff |title=GRB 150101B |url=http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=GRB+150101B |date=17 October 2018 |work=SIMBAD |accessdate=17 October 2018 }} in the constellation Virgo. The characteristics of GRB 150101B are remarkably similar to those of historic event GW170817, known to be a merger of two neutron stars.

Observations

In October 2018, astronomers reported that GRB 150101B, 1.7 billion light years away from Earth, may be analogous to the historic GW170817, a gravitational wave detected in 2017, which is about 130 million light years away, and associated with the merger of two neutron stars. The similarities between the two events, in terms of gamma ray, optical and x-ray emissions, as well as to the nature of the associated host galaxies, are considered "striking", and this remarkable resemblance suggests the two separate and independent events may both be the result of the merger of neutron stars, and both may be a hitherto-unknown class of kilonova transients. Kilonova events, therefore, may be more diverse and common in the universe than previously understood, according to the researchers.{{cite web |author=Staff |title=All in the Family: Kin of Gravitational-Wave Source Discovered |url=http://chandra.harvard.edu/photo/2018/kilonova/ |date=16 October 2018 |work=Harvard University |accessdate=17 October 2018}}{{cite news |author=University of Maryland |title=All in the family: Kin of gravitational wave source discovered - New observations suggest that kilonovae -- immense cosmic explosions that produce silver, gold and platinum--may be more common than thought |url=https://www.eurekalert.org/pub_releases/2018-10/uom-ait101518.php |date=16 October 2018 |work=EurekAlert! |accessdate=17 October 2018 |author-link=University of Maryland }}{{cite journal |author=Troja, E.|display-authors=etal |title=A luminous blue kilonova and an off-axis jet from a compact binary merger at z = 0.1341 |date=16 October 2018 |journal=Nature Communications |volume=9 |pages=4089 |number=4089 (2018) |doi=10.1038/s41467-018-06558-7 |pmid=30327476 |pmc=6191439 |bibcode=2018NatCo...9.4089T |arxiv=1806.10624 }}{{cite news |last=Mohon |first=Lee |title=GRB 150101B: A Distant Cousin to GW170817 |url=https://www.nasa.gov/mission_pages/chandra/images/grb-150101b-a-distant-cousin-to-gw170817.html |date=16 October 2018 |work=NASA |accessdate=17 October 2018 }}{{cite web |last=Wall |first=Mike |title=Powerful Cosmic Flash Is Likely Another Neutron-Star Merger |url=https://www.space.com/42158-another-neutron-star-crash-detected.html |date=17 October 2018 |work=Space.com |accessdate=17 October 2018 }}

According to one of the study researchers, Eleonora Troja, "It's a big step to go from one detected object to two. Our discovery tells us that events like GW170817 and GRB 150101B could represent a whole new class of erupting objects that turn on and off in X-rays and might actually be relatively common."{{cite news |author=Staff |title=Astronomers Find Object with Remarkable Similarities to Neutron-Star Merger GW170817 |url=http://www.sci-news.com/astronomy/kilonova-grb-150101b-06512.html |date=17 October 2018 |work=Sci-News.com |accessdate=17 October 2018 }} Troja further stated, "We've been able [to] identify this kilonova without gravitational wave data, so maybe in the future, we'll even be able to do this without directly observing a gamma-ray burst."{{cite web |last=Klesman |first=Alison |title=Another neutron star merger may have been spotted - An event that looks suspiciously like the one that produced gravitational waves in 2017 hints that mergers between neutron stars and other exotic objects may be easier to find than we'd thought. |url=http://astronomy.com/news/2018/10/a-second-neutron-star-merger-may-have-been-spotted |date=17 October 2018 |work=Astronomy |accessdate=17 October 2018 }} Another researcher, Geoffrey Ryan, said, "We have a case of cosmic look-alikes. They look the same, act the same and come from similar neighborhoods, so the simplest explanation is that they are from the same family of objects." According to co-author, Alexander Kutyrev, "If the next such observation reveals a merger between a neutron star and a black hole, that would be truly groundbreaking. Our latest observations give us renewed hope that we'll see such an event before too long." Another researcher, Hendrik Van Eerten, noted, "We need more cases like GW170817 that combine gravitational wave and electromagnetic data to find an example between a neutron star and black hole. Such a detection would be the first of its kind. Our results are encouraging for finding more mergers and making such a detection."

See also

References

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