Log in

Relevant bibliographies by topics / Supernova 1987A / Journal articles

To see the other types of publications on this topic, follow the link: Supernova 1987A.

Journal articles on the topic 'Supernova 1987A'

Author: Grafiati

Published: 4 June 2021

Last updated: 21 February 2023

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the top 50 journal articles for your research on the topic 'Supernova 1987A.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Browse journal articles on a wide variety of disciplines and organise your bibliography correctly.

1

Diodato, Virgil. "Supernova 1987A." Science & Technology Libraries 11, no. 2 (1991): 101–37. http://dx.doi.org/10.1300/j122v11n02_09.

Full text

APA, Harvard, Vancouver, ISO, and other styles

2

Arnett, W. David, John N. Bahcall, Robert P. Kirshner, and Stanford E. Woosley. "Supernova 1987A." Annual Review of Astronomy and Astrophysics 27, no. 1 (1989): 629–700. http://dx.doi.org/10.1146/annurev.aa.27.090189.003213.

Full text

APA, Harvard, Vancouver, ISO, and other styles

3

WOOSLEY, S. E., and M. M. PHILLIPS. "Supernova 1987A!" Science 240, no. 4853 (1988): 750–59. http://dx.doi.org/10.1126/science.240.4853.750.

Full text

APA, Harvard, Vancouver, ISO, and other styles

4

Fu, Albert. "Simple Perspectives on SN 1987A." Publications of the Astronomical Society of Australia 7, no. 4 (1988): 505–12. http://dx.doi.org/10.1017/s1323358000022700.

Full text

Abstract:

AbstractThis conference has shown that the accumulated wealth of data on SN 1987A has enabled us to learn an unprecedented amount of physical information about a single supernova event and supernovae in general, as well as to confirm much of the heretofore established theory. While some difficult problems remain, I discuss some particularly simple and useful theoretical notions concerning the bolometric and γ-ray light curves which can be gleaned from our current body of knowledge, drawing primarily upon results of analytic work performed by W.D. Arnett and myself. Also, the work of Lamb, Meli

APA, Harvard, Vancouver, ISO, and other styles

5

Arnett, W. David. "Supernova theory and supernova 1987A." Astrophysical Journal 319 (August 1987): 136. http://dx.doi.org/10.1086/165439.

Full text

APA, Harvard, Vancouver, ISO, and other styles

6

Nomoto, K., T. Shigeyama, and T. Tsujimoto. "Supernova Abundance Generation." Symposium - International Astronomical Union 145 (1991): 21–38. http://dx.doi.org/10.1017/s007418090022723x.

Full text

Abstract:

Theoretical models of supernova explosions of various types are reviewed to obtain heavy element yields from supernovae. We focus on new models for SN 1987A, and Type Ia, Ib, and Ic supernovae. Maximum brightness and decline rate of their light curves suggest that 12–18 M⊙ stars produce larger amount of 56Ni than more massive stars. We discuss relative roles of various types of supernovae in the chemical evolution of galaxies.

APA, Harvard, Vancouver, ISO, and other styles

7

McCray, Richard, J. Michael Shull, and Peter Sutherland. "Inside supernova 1987A." Astrophysical Journal 317 (June 1987): L73. http://dx.doi.org/10.1086/184915.

Full text

APA, Harvard, Vancouver, ISO, and other styles

8

McCray, Richard. "Supernova 1987A Revisited." Annual Review of Astronomy and Astrophysics 31, no. 1 (1993): 175–216. http://dx.doi.org/10.1146/annurev.aa.31.090193.001135.

Full text

APA, Harvard, Vancouver, ISO, and other styles

9

Kirshner, Robert P. "Supernova Remnants and their Supernovae." International Astronomical Union Colloquium 101 (1988): 1–14. http://dx.doi.org/10.1017/s0252921100102027.

Full text

Abstract:

AbstractObserving supernova remnants provides important clues to the nature of supernova explosions. Conversely, the late stages of stellar evolution and the mechanism of supernova explosions affect supernova remnants through circumstellar matter, stellar remnants, and nucleosynthesis. The elements of supernova classification and the connection between supernova type and remnant properties are explored. A special emphasis is placed on SN 1987a which provides a unique opportunity to learn the connection between the star that exploded (whose name we know) and the remnant that will develop in our

APA, Harvard, Vancouver, ISO, and other styles

10

Matsuura, M., E. Dwek, M. Meixner, et al. "Herschel Detects a Massive Dust Reservoir in Supernova 1987A." Science 333, no. 6047 (2011): 1258–61. http://dx.doi.org/10.1126/science.1205983.

Full text

Abstract:

We report far-infrared and submillimeter observations of supernova 1987A, the star whose explosion was observed on 23 February 1987 in the Large Magellanic Cloud, a galaxy located 160,000 light years away. The observations reveal the presence of a population of cold dust grains radiating with a temperature of about 17 to 23 kelvin at a rate of about 220 times the luminosity of the Sun. The intensity and spectral energy distribution of the emission suggest a dust mass of about 0.4 to 0.7 times the mass of the Sun. The radiation must originate from the supernova ejecta and requires the efficient

APA, Harvard, Vancouver, ISO, and other styles

11

RAYCHAUDHURI, PROBHAS, and DIPTIMAN SAHA. "SUBMILLISECOND PERIOD IN SUPERNOVA 1987A NEUTRINO DATA." Modern Physics Letters A 05, no. 01 (1990): 61–66. http://dx.doi.org/10.1142/s021773239000007x.

Full text

Abstract:

The neutrino burst from supernova 1987A detected by Mont Blanc, Kamiokande, IMB and Baksan have been studied within 0.01 ms to 1 ms by Ferraz-Mello technique to find periods from uneven spaced data. It is found that only Kamiokande and IMB neutrino data have significant periods 0.499 ms and 0.568 ms, respectively. Our analysis suggest that the supernova 1987A contains a submillisecond pulsar and is supported by the recently discovered submillisecond period detected from supernova 1987A optical data. We suggest that the pulsar in supernova 1987A is a radially pulsating neutron star.

APA, Harvard, Vancouver, ISO, and other styles

12

Panagia, Nino. "SUPERNOVA 1987A: CELEBRATING A SILVER JUBILEE." Acta Polytechnica 53, A (2013): 606–11. http://dx.doi.org/10.14311/ap.2013.53.0606.

Full text

Abstract:

The story of the SN 1987A explosion is briefly reviewed. Although this supernova was somewhat peculiar, the study of SN 1987A has clarified quite a number of important aspects of the nature and the properties of supernovae, such as the confirmation of the core collapse of a massive star as the cause of the explosion, as well the confirmation that the decays 56Ni–56Co–56Fe at early times and 44Ti–44Sc at late times, are the main sources of the energy radiated by the ejecta. Still we have not been able to ascertain whether the progenitor was a single star or a binary system, nor have we been abl

APA, Harvard, Vancouver, ISO, and other styles

13

Thomsen, D. E. "Supernova 1987A: Astronomers' Luck." Science News 131, no. 10 (1987): 148. http://dx.doi.org/10.2307/3971435.

Full text

APA, Harvard, Vancouver, ISO, and other styles

14

Leising, M. D. "55Fe in Supernova 1987A." Astrophysical Journal 651, no. 2 (2006): 1019–22. http://dx.doi.org/10.1086/507602.

Full text

APA, Harvard, Vancouver, ISO, and other styles

15

PIRAN, Tsvi, and TAKASHI NAKAMURA. "Jets in supernova 1987A?" Nature 330, no. 6143 (1987): 28. http://dx.doi.org/10.1038/330028b0.

Full text

APA, Harvard, Vancouver, ISO, and other styles

16

Milone, Luis A., S. Paolantonio, V. Briggi, D. Mendicini, and E. Minniti. "The unusual supernova 1987A." Astrophysics and Space Science 150, no. 2 (1988): 291–97. http://dx.doi.org/10.1007/bf00641723.

Full text

APA, Harvard, Vancouver, ISO, and other styles

17

Wilson, J. "Neutrinos and supernova 1987a." Nuclear Physics B - Proceedings Supplements 13 (February 1990): 380–82. http://dx.doi.org/10.1016/0920-5632(90)90091-8.

Full text

APA, Harvard, Vancouver, ISO, and other styles

18

Kahana, S. H., J. Cooperstein, and E. Baron. "Neutrinos from supernova 1987A." Physics Letters B 196, no. 3 (1987): 259–66. http://dx.doi.org/10.1016/0370-2693(87)90727-1.

Full text

APA, Harvard, Vancouver, ISO, and other styles

19

Joss, P. C. "Type II Supernovae in Binary Systems." Symposium - International Astronomical Union 165 (1996): 141–49. http://dx.doi.org/10.1017/s0074180900055637.

Full text

Abstract:

The presence of a close binary companion can affect the evolution of a massive star through one or more episodes of mass transfer, or by merger in a common-envelope phase. Monte Carlo calculations indicate that ∼20–35% of all massive supernovae are affected by such processes, and that a substantial fraction of these events will be supernovae of type II. The properties of the progenitor star, the distribution of circumstellar material, the peak supernova luminosity, the shape of the supernova light curve, and other observable features of the supernova event can be affected by prior binary membe

APA, Harvard, Vancouver, ISO, and other styles

20

KRIVOSHEINA, I. V. "SN 1987A — HISTORICAL VIEW ABOUT REGISTRATION OF THE NEUTRINO SIGNAL WITH BAKSAN, KAMIOKANDE II AND IMB DETECTORS." International Journal of Modern Physics D 13, no. 10 (2004): 2085–105. http://dx.doi.org/10.1142/s0218271804006607.

Full text

Abstract:

The detection of neutrinos from SN 1987A opened a new era in neutrino astrophysics in the last century. We present a historical view about registration of the neutrino signal from supernova SN 1987A in the Large Magellanic Cloud by the BAKSAN liquid scintillator detector and by the two water Cherenkov detectors — Kamiokande-II and IMB. All three detectors observed a total neutrino signal of 24 events at 7:35 UT 23 February, 1987. I will concentrate mostly about the BAKSAN supernova group analysis of the neutrino signal, which was already done in the years 1987 and 1988. The results of this ana

APA, Harvard, Vancouver, ISO, and other styles

21

McCray, Richard. "Supernova 1987A: The Birth of a Supernova Remnant." International Astronomical Union Colloquium 192 (2005): 77–87. http://dx.doi.org/10.1017/s0252921100009027.

Full text

APA, Harvard, Vancouver, ISO, and other styles

22

Dwek, Eli. "Infrared Emission from Dust in Supernovae and Supernova Remnants." Symposium - International Astronomical Union 135 (1989): 479–86. http://dx.doi.org/10.1017/s0074180900125471.

Full text

Abstract:

The need to replenish the reservoir of interstellar dust grains that are continuously being destroyed in the interstellar medium, and the presence of isotopic anomalies in meteorites, suggest that supernovae may be important sources of interstellar dust. Infrared observations of supernovae or their unmixed ejecta may provide the first direct evidence for newly-formed grains in this environment. The recently discovered supernova, SN 1987A, currently offers the best prospects for observing the actual process of dust formation in a supernova.In contrast, supernova remnants constitute the most imp

APA, Harvard, Vancouver, ISO, and other styles

23

Waldrop, M. Mitchell. "The Supernova 1987A Pulsar: Found?" Science 243, no. 4893 (1989): 892. http://dx.doi.org/10.1126/science.243.4893.892.a.

Full text

APA, Harvard, Vancouver, ISO, and other styles

24

Roche, P. F., D. K. Aitken, and C. H. Smith. "Silicon monoxide in Supernova 1987A." Monthly Notices of the Royal Astronomical Society 252, no. 1 (1991): 39P—42P. http://dx.doi.org/10.1093/mnras/252.1.39p.

Full text

APA, Harvard, Vancouver, ISO, and other styles

25

Podsiadlowski, Ph. "Running rings around supernova 1987A." Nature 350, no. 6320 (1991): 654–55. http://dx.doi.org/10.1038/350654a0.

Full text

APA, Harvard, Vancouver, ISO, and other styles

26

Sato, H. "Pulsar Nebula and Supernova 1987A." Progress of Theoretical Physics 80, no. 1 (1988): 96–107. http://dx.doi.org/10.1143/ptp.80.96.

Full text

APA, Harvard, Vancouver, ISO, and other styles

27

McCray, Richard, and Claes Fransson. "The Remnant of Supernova 1987A." Annual Review of Astronomy and Astrophysics 54, no. 1 (2016): 19–52. http://dx.doi.org/10.1146/annurev-astro-082615-105405.

Full text

APA, Harvard, Vancouver, ISO, and other styles

28

Spyromilio, J., W. P. S. Meikle, R. C. M. Learner, and D. A. Allen. "Carbon monoxide in supernova 1987A." Nature 334, no. 6180 (1988): 327–29. http://dx.doi.org/10.1038/334327a0.

Full text

APA, Harvard, Vancouver, ISO, and other styles

29

Riegler, G. R. "Observations of supernova SN 1987A." IEEE Transactions on Nuclear Science 35, no. 1 (1988): 516–19. http://dx.doi.org/10.1109/23.12776.

Full text

APA, Harvard, Vancouver, ISO, and other styles

30

Galeotti, P., and G. Pizzella. "Supernova 1987A, 30 Years Later." Physics of Atomic Nuclei 81, no. 1 (2018): 105–12. http://dx.doi.org/10.1134/s1063778818010106.

Full text

APA, Harvard, Vancouver, ISO, and other styles

31

Krauss, Lawrence M. "Neutrino spectroscopy of supernova 1987A." Nature 329, no. 6141 (1987): 689–94. http://dx.doi.org/10.1038/329689a0.

Full text

APA, Harvard, Vancouver, ISO, and other styles

32

Lindley, David. "Supernova 1987A: one year old." Nature 331, no. 6157 (1988): 567. http://dx.doi.org/10.1038/331567a0.

Full text

APA, Harvard, Vancouver, ISO, and other styles

33

Fang, Lizhi. "Neutrino mass and supernova 1987a." Chinese Physics Letters 4, no. 9 (1987): 424–26. http://dx.doi.org/10.1088/0256-307x/4/9/011.

Full text

APA, Harvard, Vancouver, ISO, and other styles

34

Staveley-Smith, L., T. M. Potter, G. Zanardo, B. M. Gaensler, and C. Y. Ng. "Radio Observations of Supernova 1987A." Proceedings of the International Astronomical Union 9, S296 (2013): 15–22. http://dx.doi.org/10.1017/s1743921313009174.

Full text

Abstract:

AbstractSupernovae and their remnants are believed to be prodigious sources of Galactic cosmic rays and interstellar dust. Understanding the mechanisms behind their surprisingly high production rate is helped by the study of nearby young supernova remnants. There has been none better in modern times than SN1987A, for which radio observations have been made for over a quarter of a century. We review extensive observations made with the Australia Telescope Compact Array (ATCA) at centimetre wavelengths. Emission at frequencies from 1 to 100 GHz is dominated by synchrotron radiation from an outer

APA, Harvard, Vancouver, ISO, and other styles

35

Sonneborn, George, C. S. J. Pun, Peter Garnavich, and Robert Kirshner. "Birth of Supernova Remnant 1987A." Symposium - International Astronomical Union 190 (1999): 136–38. http://dx.doi.org/10.1017/s0074180900117656.

Full text

APA, Harvard, Vancouver, ISO, and other styles

36

Shapiro, I., N. Bartel, R. Preston, et al. "VLBI Observations of Supernova 1987A." Symposium - International Astronomical Union 129 (1988): 185–86. http://dx.doi.org/10.1017/s0074180900134436.

Full text

Abstract:

VLBI observations at 2.3 GHz of SN1987A on 28 February 1987 yielded no fringes, implying, for an optically thin shell, a lower bound on the (outer) diameter of 1.9 mas. From the comparison of the VLBI and optical results, we infer that the radiosphere of SN1987A was either about equal to, or larger than, the photosphere of the supernova five days after the explosion.

APA, Harvard, Vancouver, ISO, and other styles

37

Schramm, D. "New physics from supernova 1987A." Physics Reports 189, no. 2 (1990): 89–126. http://dx.doi.org/10.1016/0370-1573(90)90020-3.

Full text

APA, Harvard, Vancouver, ISO, and other styles

38

Schramm, David N. "A look at supernova 1987A." Nuclear Physics B - Proceedings Supplements 3 (March 1988): 471–93. http://dx.doi.org/10.1016/0920-5632(88)90198-3.

Full text

APA, Harvard, Vancouver, ISO, and other styles

39

Barkat, Zalman, and J. Craig Wheeler. "Supernova 1987A - The progenitor corridor." Astrophysical Journal 341 (June 1989): 925. http://dx.doi.org/10.1086/167550.

Full text

APA, Harvard, Vancouver, ISO, and other styles

40

Woosley, S. E., Philip A. Pinto, and L. Ensman. "Supernova 1987A - Six weeks later." Astrophysical Journal 324 (January 1988): 466. http://dx.doi.org/10.1086/165908.

Full text

APA, Harvard, Vancouver, ISO, and other styles

41

Xu, Yueming, Peter Sutherland, Richard McCray, and Randy R. Ross. "X-rays from supernova 1987A." Astrophysical Journal 327 (April 1988): 197. http://dx.doi.org/10.1086/166181.

Full text

APA, Harvard, Vancouver, ISO, and other styles

42

WALDROP, M. MITCHELL. "Supernova 1987A: Facts and Fancies." Science 239, no. 4839 (1988): 460–62. http://dx.doi.org/10.1126/science.239.4839.460.

Full text

APA, Harvard, Vancouver, ISO, and other styles

43

Sharp, C. M., and P. H�flich. "Molecular bands of supernova 1987A." Astrophysics and Space Science 171, no. 1-2 (1990): 213–16. http://dx.doi.org/10.1007/bf00646849.

Full text

APA, Harvard, Vancouver, ISO, and other styles

44

Meaburn, J., M. Bryce, and A. J. Holloway. "Smoke rings around supernova 1987a." Astrophysics and Space Science 233, no. 1-2 (1995): 75–79. http://dx.doi.org/10.1007/bf00627336.

Full text

APA, Harvard, Vancouver, ISO, and other styles

45

Orlando, S., M. Miceli, M. L. Pumo, and F. Bocchino. "SUPERNOVA 1987A: A TEMPLATE TO LINK SUPERNOVAE TO THEIR REMNANTS." Astrophysical Journal 810, no. 2 (2015): 168. http://dx.doi.org/10.1088/0004-637x/810/2/168.

Full text

APA, Harvard, Vancouver, ISO, and other styles

46

Turtle, A. J., D. Campbell-Wilson, J. D. Bunton, et al. "Initial Radio Observations of SN1987a in the Large Magellanic Cloud." Symposium - International Astronomical Union 129 (1988): 189. http://dx.doi.org/10.1017/s007418090013445x.

Full text

Abstract:

A prompt radio burst has been observed from the supernova 1987a in the Large Magellanic Cloud. Observations were made at 0.843, 1.415, 2.29, and 8.41 GHz. At frequencies around 1 GHz, the peak flux density reached about 150 mJy and occurred within four days of the supernova. This event may be a weak precursor to a major radio outburst of the type previously observed in other extragalactic supernovae. Radio monitoring of the supernova is continuing at each of the above frequencies, and coordination is underway of a southern hemisphere VLBI array to map the radio outburst region as it expands. D

APA, Harvard, Vancouver, ISO, and other styles

47

Sood, R. K., J. A. Thomas, L. Waldron та ін. "High Energy γ-ray Observations of SN 1987A". Publications of the Astronomical Society of Australia 7, № 4 (1988): 486–89. http://dx.doi.org/10.1017/s1323358000022682.

Full text

Abstract:

AbstractSN 1987A has been observed with a combined high energy γ-ray (50-500 MeV) and hard X-ray (15-150 keV) payload during a balloon flight on 5 April 1988 from Alice Springs, Australia. The γ-ray observations, along with our earlier ones on 19 April 1987 are the only such observations of the supernova to date. The γ-ray detector characteristics are described. The preliminary results of the recent flight and their implications in terms of the known supernova parameters are discussed.

APA, Harvard, Vancouver, ISO, and other styles

48

Spyromilio, Jason. "Infrared Spectroscopy of SN 1987A." International Astronomical Union Colloquium 145 (1996): 193–99. http://dx.doi.org/10.1017/s025292110000806x.

Full text

Abstract:

Infrared spectra of SN 1987A have been obtained at the Anglo-Australian Telescope since the explosion of this supernova. I present highlights from this program which include the analysis of the molecular emission, the determination of the mass of 57Co in the ejecta and the analysis of the emission due to dust in the ejecta. I also show the spectrum of the supernova in the infrared 5 years after explosion.

APA, Harvard, Vancouver, ISO, and other styles

49

Staveley-Smfth, L., R. N. Manchester, M. J. Kesteven, et al. "Birth of a radio supernova remnant in supernova 1987A." Nature 355, no. 6356 (1992): 147–49. http://dx.doi.org/10.1038/355147a0.

Full text

APA, Harvard, Vancouver, ISO, and other styles

50

Kotak, Rubina. "Core-Collapse Supernovae as Dust Producers." Proceedings of the International Astronomical Union 3, S250 (2007): 437–42. http://dx.doi.org/10.1017/s1743921308020802.

Full text

Abstract:

AbstractAlthough it has long been hypothesised that core-collapse supernovae may produce large quantities of dust, interest in this problem has recently been rekindled given the enormous dust masses inferred at very high redshifts (z ≳ 6), when conventional low-mass dust-producing stars would fail to contribute significantly to the universal dust budget. Emission due to warm dust peaks at mid-IR wavelengths. However, with the notable exception of SN 1987A, supernova studies in the mid-IR have been virtually non-existent until the advent of the Spitzer Space Telescope. On behalf of the Mid-Infr

APA, Harvard, Vancouver, ISO, and other styles

We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!