Nuclear star formation in the hot-spot galaxy HGC 2903

A. Alonso-Herrero; S.D. Ryder; J. Knapen

doi:10.1046/j.1365-8711.2001.04173.x

Nuclear star formation in the hot-spot galaxy HGC 2903

A. Alonso-Herrero, S.D. Ryder, J. Knapen

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Abstract

Circumnuclear regions (CNR) of enhanced star formation (SF) in disk galaxies are usually associated with the presence of stellar bars. Since bars are believed to be one of the most effective mechanisms for transporting material into the central regions of galaxies, CNRs are excellent laboratories for the study of the effects of inflow processes on the triggering of SF (see Knapen 1999 for a review on the subject).

Original language	English
Pages (from-to)	16-17
Journal	Canada-France-Hawaii Telescope Information Bulletin
Volume	42
DOIs	https://doi.org/10.1046/j.1365-8711.2001.04173.x
Publication status	Published - Jun 2000

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title = "Nuclear star formation in the hot-spot galaxy HGC 2903",

abstract = "Circumnuclear regions (CNR) of enhanced star formation (SF) in disk galaxies are usually associated with the presence of stellar bars. Since bars are believed to be one of the most effective mechanisms for transporting material into the central regions of galaxies, CNRs are excellent laboratories for the study of the effects of inflow processes on the triggering of SF (see Knapen 1999 for a review on the subject).",

author = "A. Alonso-Herrero and S.D. Ryder and J. Knapen",

note = "Original article can be found at : http://www.cfht.hawaii.edu/Reference/Bulletin/",

year = "2000",

month = jun,

doi = "10.1046/j.1365-8711.2001.04173.x",

language = "English",

volume = "42",

pages = "16--17",

journal = "Canada-France-Hawaii Telescope Information Bulletin",

publisher = "Institute of Astronomy and Astrophysics, Academia Sinica",

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TY - JOUR

T1 - Nuclear star formation in the hot-spot galaxy HGC 2903

AU - Alonso-Herrero, A.

AU - Ryder, S.D.

AU - Knapen, J.

N1 - Original article can be found at : http://www.cfht.hawaii.edu/Reference/Bulletin/

PY - 2000/6

Y1 - 2000/6

N2 - Circumnuclear regions (CNR) of enhanced star formation (SF) in disk galaxies are usually associated with the presence of stellar bars. Since bars are believed to be one of the most effective mechanisms for transporting material into the central regions of galaxies, CNRs are excellent laboratories for the study of the effects of inflow processes on the triggering of SF (see Knapen 1999 for a review on the subject).

AB - Circumnuclear regions (CNR) of enhanced star formation (SF) in disk galaxies are usually associated with the presence of stellar bars. Since bars are believed to be one of the most effective mechanisms for transporting material into the central regions of galaxies, CNRs are excellent laboratories for the study of the effects of inflow processes on the triggering of SF (see Knapen 1999 for a review on the subject).

U2 - 10.1046/j.1365-8711.2001.04173.x

DO - 10.1046/j.1365-8711.2001.04173.x

M3 - Article

VL - 42

SP - 16

EP - 17

JO - Canada-France-Hawaii Telescope Information Bulletin

JF - Canada-France-Hawaii Telescope Information Bulletin

ER -

Nuclear star formation in the hot-spot galaxy HGC 2903

Abstract

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