Search Results - "Shara, M. M."
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GROWING WHITE DWARFS TO THE CHANDRASEKHAR LIMIT: THE PARAMETER SPACE OF THE SINGLE DEGENERATE SN Ia CHANNEL
Published in The Astrophysical journal (10-03-2016)“…ABSTRACT Can a white dwarf (WD), accreting hydrogen-rich matter from a non-degenerate companion star, ever exceed the Chandrasekhar mass and explode as a SN…”
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Observational signatures of SNIa progenitors, as predicted by models
Published in Monthly notices of the Royal Astronomical Society (11-01-2015)“…A definitive determination of the progenitors of Type Ia supernovae (SNIa) has been a conundrum for decades. The single degenerate scenario -- a white dwarf…”
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Mussel-Inspired Surface Chemistry for Multifunctional Coatings
Published in Science (American Association for the Advancement of Science) (19-10-2007)“…We report a method to form multifunctional polymer coatings through simple dip-coating of objects in an aqueous solution of dopamine. Inspired by the…”
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Forced degradation of recombinant monoclonal antibodies: A practical guide
Published in mAbs (17-11-2017)“…Forced degradation studies have become integral to the development of recombinant monoclonal antibody therapeutics by serving a variety of objectives from…”
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Possible Detection of the Progenitor of the Type II Supernova SN 2023ixf
Published in Astrophysical journal. Letters (01-08-2023)“…Abstract Stellar evolution theory predicts multiple pathways to the explosive deaths of stars as supernovae. Locating and characterizing the progenitors of…”
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The Massive CO White Dwarf in the Symbiotic Recurrent Nova RS Ophiuchi
Published in The Astrophysical journal (01-10-2017)“…If accreting white dwarfs (WDs) in binary systems are to produce type Ia supernovae (SNe Ia), they must grow to nearly the Chandrasekhar mass and ignite carbon…”
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M31N 2008-12a-THE REMARKABLE RECURRENT NOVA IN M31: PANCHROMATIC OBSERVATIONS OF THE 2015 ERUPTION
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT The Andromeda Galaxy recurrent nova M31N 2008-12a had been observed in eruption 10 times, including yearly eruptions from 2008 to 2014. With a…”
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An Extended Grid of Nova Models. II. The Parameter Space of Nova Outbursts
Published in The Astrophysical journal (10-04-2005)“…This paper is a sequel to an earlier paper devoted to multiple, multicycle nova evolution models (Prialnik & Kovetz, Paper I), which showed that the different…”
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DYNAMICAL INTERACTIONS MAKE HOT JUPITERS IN OPEN STAR CLUSTERS
Published in The Astrophysical journal (10-01-2016)“…ABSTRACT Explaining the origin and evolution of exoplanetary hot Jupiters remains a significant challenge. One possible mechanism for the production of hot…”
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Inflows, Outflows, and a Giant Donor in the Remarkable Recurrent Nova M31N 2008-12a?-Hubble Space Telescope Photometry of the 2015 Eruption
Published in The Astrophysical journal (10-11-2017)“…The recurrent nova M31N 2008-12a experiences annual eruptions, contains a near-Chandrasekhar-mass white dwarf, and has the largest mass accretion rate in any…”
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Laparoscopic endoloop excision of non-communicating rudimentary uterine horn ectopic pregnancy in the first trimester
Published in American journal of obstetrics and gynecology (25-10-2024)Get full text
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On an apparent dearth of recurrent nova super-remnants in the Local Group
Published in Monthly notices of the Royal Astronomical Society (01-02-2024)“…ABSTRACT The Andromeda Galaxy is home to the annually erupting recurrent nova (RN) M 31N 2008-12a (12a); the first nova found to host a nova super-remnant…”
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Proper-motion age dating of the progeny of Nova Scorpii AD 1437
Published in Nature (London) (31-08-2017)“…The re-discovery of the binary star system that created the Nova Scorpii AD 1437 stellar outburst shows that it is now a dwarf nova, suggesting that nova…”
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Revised Metallicity Classes for Low-Mass Stars: Dwarfs (dM), Subdwarfs (sdM), Extreme Subdwarfs (esdM), and Ultrasubdwarfs (usdM)
Published in The Astrophysical journal (10-11-2007)“…The current classification system of M stars on the main sequence distinguishes three metallicity classes (dwarfs: dM; subdwarfs: sdM; and extreme subdwarfs:…”
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A 9 Month Hubble Space Telescope Near-UV Survey of M87. II. A Strongly Enhanced Nova Rate near the Jet of M87
Published in The Astrophysical journal (01-10-2024)“…Abstract The 135 classical novae that we have discovered in M87 with two Hubble Space Telescope imaging surveys appear to be strongly concentrated along that…”
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Improving the interpretation of electronic fetal monitoring: the fetal reserve index
Published in American journal of obstetrics and gynecology (01-05-2023)“…Electronic fetal monitoring, particularly in the form of cardiotocography, forms the centerpiece of labor management. Initially successfully designed for…”
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PAN-CHROMATIC OBSERVATIONS OF THE RECURRENT NOVA LMC 2009a (LMC 1971b)
Published in The Astrophysical journal (20-02-2016)“…ABSTRACT Nova LMC 2009a is confirmed as a recurrent nova (RN) from positional coincidence with nova LMC 1971b. The observational data set is one of the most…”
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An age difference of two billion years between a metal-rich and a metal-poor globular cluster
Published in Nature (London) (01-08-2013)“…An absolute age of about ten billion years is determined for the globular cluster 47 Tucanae, which is about two billion years younger than the cluster NGC…”
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A recurrent nova super-remnant in the Andromeda galaxy
Published in Nature (London) (01-01-2019)“…The accretion of hydrogen onto a white dwarf star ignites a classical nova eruption 1 , 2 —a thermonuclear runaway in the accumulated envelope of gas, leading…”
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The symbiotic recurrent nova V3890 Sgr: binary parameters and pre-outburst activity
Published in Monthly notices of the Royal Astronomical Society (01-06-2021)“…ABSTRACT We present and analyse optical photometry and high-resolution Southern African Large Telescope spectra of the symbiotic recurrent nova V3890 Sgr at…”
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