Erratum: Are the ultra-faint dwarf galaxies just cusps? (The Astrophysical Journal Letters (2011) 727 (L14))

Adi Zolotov; David W. Hogg; Beth Willman

doi:10.1088/2041-8205/732/2/L37

Erratum: Are the ultra-faint dwarf galaxies just cusps? (The Astrophysical Journal Letters (2011) 727 (L14))

Adi Zolotov, David W. Hogg, Beth Willman

Research output: Contribution to journal › Comment/debate › peer-review

Original language	English (US)
Article number	L37
Journal	Astrophysical Journal Letters
Volume	732
Issue number	2 PART II
DOIs	https://doi.org/10.1088/2041-8205/732/2/L37
State	Published - May 10 2011

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

Access to Document

10.1088/2041-8205/732/2/L37

Cite this

@article{df40c5124a8f4961a3f68419d5a8f88f,

title = "Erratum: Are the ultra-faint dwarf galaxies just cusps? (The Astrophysical Journal Letters (2011) 727 (L14))",

author = "Adi Zolotov and Hogg, {David W.} and Beth Willman",

year = "2011",

month = may,

day = "10",

doi = "10.1088/2041-8205/732/2/L37",

language = "English (US)",

volume = "732",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "IOP Publishing Ltd.",

number = "2 PART II",

}

TY - JOUR

T1 - Erratum

T2 - Are the ultra-faint dwarf galaxies just cusps? (The Astrophysical Journal Letters (2011) 727 (L14))

AU - Zolotov, Adi

AU - Hogg, David W.

AU - Willman, Beth

PY - 2011/5/10

Y1 - 2011/5/10

UR - http://www.scopus.com/inward/record.url?scp=79955578076&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=79955578076&partnerID=8YFLogxK

U2 - 10.1088/2041-8205/732/2/L37

DO - 10.1088/2041-8205/732/2/L37

M3 - Comment/debate

AN - SCOPUS:79955578076

SN - 2041-8205

VL - 732

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2 PART II

M1 - L37

ER -

Erratum: Are the ultra-faint dwarf galaxies just cusps? (The Astrophysical Journal Letters (2011) 727 (L14))

ASJC Scopus subject areas

Access to Document

Other files and links

Cite this