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Search: WFRF:(Lunnan Ragnhild) > iPTF 16hgs :

iPTF 16hgs : A Double-peaked Ca-rich Gap Transient in a Metal-poor, Star-forming Dwarf Galaxy

De, Kishalay (author)
CALTECH, Cahill Ctr Astrophys, 1200 East Calif Blvd, Pasadena, CA 91125 USA
Kasliwal, Mansi M. (author)
CALTECH, Cahill Ctr Astrophys, 1200 East Calif Blvd, Pasadena, CA 91125 USA
Cantwell, Therese (author)
Univ Manchester, Jodrell Bank Ctr Astrophys, Sch Phys & Astron, Alan Turing Bldg,Oxford Rd, Manchester M13 9PL, Lancs, England
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Cao, Yi (author)
Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA
Cenko, S. Bradley (author)
NASA, Astrophys Sci Div, Goddard Space Flight Ctr, Mail Code 661, Greenbelt, MD 20771 USA;Univ Maryland, Joint Space Sci Inst, College Pk, MD 20742 USA
Gal-Yam, Avishay (author)
Weizmann Inst Sci, Dept Particle Phys & Astrophys, Fac Phys, IL-76100 Rehovot, Israel
Johansson, Joel, Dr, 1984- (author)
Uppsala universitet,Observationell astrofysik
Kong, Albert (author)
Natl Tsing Hua Univ, Inst Astron, Hsinchu 30013, Taiwan;Natl Tsing Hua Univ, Dept Phys, Hsinchu 30013, Taiwan
Kulkarni, Shrinivas R. (author)
CALTECH, Cahill Ctr Astrophys, 1200 East Calif Blvd, Pasadena, CA 91125 USA
Lunnan, Ragnhild (author)
Stockholms universitet,Institutionen för astronomi,Oskar Klein-centrum för kosmopartikelfysik (OKC),Stockholm Univ, Dept Astron, Oskar Klein Ctr, SE-10691 Stockholm, Sweden
Masci, Frank (author)
CALTECH, Infrared Proc & Anal Ctr, MS 100-22, Pasadena, CA 91125 USA
Matuszewski, Matt (author)
Mooley, Kunal P. (author)
CALTECH, Cahill Ctr Astrophys, 1200 East Calif Blvd, Pasadena, CA 91125 USA
Neill, James D. (author)
CALTECH, Cahill Ctr Astrophys, 1200 East Calif Blvd, Pasadena, CA 91125 USA
Nugent, Peter E. (author)
Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA;Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
Ofek, Eran O. (author)
Weizmann Inst Sci, Dept Particle Phys & Astrophys, Fac Phys, IL-76100 Rehovot, Israel
Perrott, Yvette (author)
Cavendish Lab, Astrophys Grp, 19 JJ Thomson Ave, Cambridge CB3 0HE, England
Rebbapragada, Umaa D. (author)
CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
Rubin, Adam (author)
Weizmann Inst Sci, Dept Particle Phys & Astrophys, Fac Phys, IL-76100 Rehovot, Israel
O' Sullivan, Donal (author)
CALTECH, Cahill Ctr Astrophys, 1200 East Calif Blvd, Pasadena, CA 91125 USA
Yaron, Ofer (author)
Weizmann Inst Sci, Dept Particle Phys & Astrophys, Fac Phys, IL-76100 Rehovot, Israel
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 (creator_code:org_t)
2018-10-15
2018
English.
In: Astrophysical Journal. - : American Astronomical Society. - 0004-637X .- 1538-4357. ; 866:1
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Calcium-rich gap transients represent an intriguing new class of faint and fast-evolving supernovae that exhibit strong [Ca II] emission in their nebular phase spectra. In this paper, we present the discovery and follow-up observations of a faint and fast-evolving transient, iPTF 16hgs, that exhibited a double-peaked light curve. Exhibiting a Type Ib spectrum in the photospheric phase and an early transition to a [Ca II] dominated nebular phase, iPTF 16hgs shows properties consistent with the class of Ca-rich gap transients, with two important exceptions. First, while the second peak of the light curve is similar to other Ca-rich gap transients, the first blue and fast-fading peak (declining over approximate to 2 days) is unique to this source. Second, we find that iPTF 16hgs occurred in the outskirts (projected offset of approximate to 6 kpc approximate to 1.9 R-eff) of a low-metallicity (approximate to 0.4 Z(circle dot)), star-forming, dwarf spiral galaxy. Deep limits from late-time radio observations suggest a low-density environment for the source. If iPTF 16hgs shares explosion physics with the class of Ca-rich gap transients, the first peak can be explained by the presence of 0.01 M-circle dot of Ni-56 in the outer layers the ejecta, reminiscent of some models of He-shell detonations on WDs. However, if iPTF 16hgs is physically unrelated to the class, the first peak is consistent with shock cooling emission (of an envelope with a mass of approximate to 0.08 M-circle dot and radius of approximate to 13 R-circle dot) in a core-collapse explosion of a highly stripped massive star in a close binary system.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

supernovae: general
supernovae: individual (iPTF 16hgs)
surveys

Publication and Content Type

ref (subject category)
art (subject category)

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