SN 2010U: A luminous nova in NGC 4214

Roberta M Humphreys; José L. Prieto; Philip Rosenfield; L. Andrew Helton; Christopher S. Kochanek; K. Z. Stanek; Rubab Khan; Dorota Szczygiel; Karen Mogren; Robert A. Fesen; Dan Milisavljevic; Benjamin Williams; Jeremiah Murphy; Julianne Dalcanton; Karoline Gilbert

doi:10.1088/2041-8205/718/1/L43

SN 2010U: A luminous nova in NGC 4214

Roberta M Humphreys, José L. Prieto, Philip Rosenfield, L. Andrew Helton, Christopher S. Kochanek, K. Z. Stanek, Rubab Khan, Dorota Szczygiel, Karen Mogren, Robert A. Fesen, Dan Milisavljevic, Benjamin Williams, Jeremiah Murphy, Julianne Dalcanton, Karoline Gilbert

Minnesota Institute for Astrophysics

Research output: Contribution to journal › Article › peer-review

7 Scopus citations

Abstract

The luminosity, light curve, post-maximum spectrum, and lack of a progenitor on deep pre-outburst images suggest that SN2010U was a luminous, fast nova. Its outburst magnitude is consistent with that for a fast nova using the maximum magnitude-rate of decline relationship for classical novae.

Original language	English (US)
Pages (from-to)	L43-L47
Journal	Astrophysical Journal Letters
Volume	718
Issue number	1 PART 2
DOIs	https://doi.org/10.1088/2041-8205/718/1/L43
State	Published - 2010

Keywords

novae, cataclysmic variables
stars: individual (SN 2010U)
supernovae: individual (SN 2010U)

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10.1088/2041-8205/718/1/L43

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title = "SN 2010U: A luminous nova in NGC 4214",

abstract = "The luminosity, light curve, post-maximum spectrum, and lack of a progenitor on deep pre-outburst images suggest that SN2010U was a luminous, fast nova. Its outburst magnitude is consistent with that for a fast nova using the maximum magnitude-rate of decline relationship for classical novae.",

keywords = "novae, cataclysmic variables, stars: individual (SN 2010U), supernovae: individual (SN 2010U)",

author = "Humphreys, {Roberta M} and Prieto, {Jos{\'e} L.} and Philip Rosenfield and Helton, {L. Andrew} and Kochanek, {Christopher S.} and Stanek, {K. Z.} and Rubab Khan and Dorota Szczygiel and Karen Mogren and Fesen, {Robert A.} and Dan Milisavljevic and Benjamin Williams and Jeremiah Murphy and Julianne Dalcanton and Karoline Gilbert",

year = "2010",

doi = "10.1088/2041-8205/718/1/L43",

language = "English (US)",

volume = "718",

pages = "L43--L47",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

number = "1 PART 2",

}

TY - JOUR

T1 - SN 2010U

T2 - A luminous nova in NGC 4214

AU - Humphreys, Roberta M

AU - Prieto, José L.

AU - Rosenfield, Philip

AU - Helton, L. Andrew

AU - Kochanek, Christopher S.

AU - Stanek, K. Z.

AU - Khan, Rubab

AU - Szczygiel, Dorota

AU - Mogren, Karen

AU - Fesen, Robert A.

AU - Milisavljevic, Dan

AU - Williams, Benjamin

AU - Murphy, Jeremiah

AU - Dalcanton, Julianne

AU - Gilbert, Karoline

PY - 2010

Y1 - 2010

N2 - The luminosity, light curve, post-maximum spectrum, and lack of a progenitor on deep pre-outburst images suggest that SN2010U was a luminous, fast nova. Its outburst magnitude is consistent with that for a fast nova using the maximum magnitude-rate of decline relationship for classical novae.

AB - The luminosity, light curve, post-maximum spectrum, and lack of a progenitor on deep pre-outburst images suggest that SN2010U was a luminous, fast nova. Its outburst magnitude is consistent with that for a fast nova using the maximum magnitude-rate of decline relationship for classical novae.

KW - novae, cataclysmic variables

KW - stars: individual (SN 2010U)

KW - supernovae: individual (SN 2010U)

UR - http://www.scopus.com/inward/record.url?scp=77954512287&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=77954512287&partnerID=8YFLogxK

U2 - 10.1088/2041-8205/718/1/L43

DO - 10.1088/2041-8205/718/1/L43

M3 - Article

AN - SCOPUS:77954512287

SN - 2041-8205

VL - 718

SP - L43-L47

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 1 PART 2

ER -

SN 2010U: A luminous nova in NGC 4214

Abstract

Keywords

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