CO and optical observations of the Magellanic Bridge

Francis Keenan

CO and optical observations of the Magellanic Bridge

Francis Keenan

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

Abstract

We present (CO)-C-12(1-0) molecular line and BV CCD observations towards 0311-7651: a region in the Magellanic Bridge where cold atomic Hydrogen has previously been detected by Kobulnicky & Dickey: Additionally, BV images of a comparison held 1 degrees to the South were taken. No CO was detected to a limit of similar to 0.06 Kelvin, and the colour-magnitude diagrams show no evidence for a stellar association in either field.

Original language	English
Pages (from-to)	451-454
Number of pages	4
Journal	Astronomy and Astrophysics
Volume	363
Issue number	2
Publication status	Published - 2000

ASJC Scopus subject areas

Space and Planetary Science
Astronomy and Astrophysics

Cite this

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title = "CO and optical observations of the Magellanic Bridge",

abstract = "We present (CO)-C-12(1-0) molecular line and BV CCD observations towards 0311-7651: a region in the Magellanic Bridge where cold atomic Hydrogen has previously been detected by Kobulnicky \& Dickey: Additionally, BV images of a comparison held 1 degrees to the South were taken. No CO was detected to a limit of similar to 0.06 Kelvin, and the colour-magnitude diagrams show no evidence for a stellar association in either field.",

author = "Francis Keenan",

year = "2000",

language = "English",

volume = "363",

pages = "451--454",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

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number = "2",

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T1 - CO and optical observations of the Magellanic Bridge

AU - Keenan, Francis

PY - 2000

Y1 - 2000

N2 - We present (CO)-C-12(1-0) molecular line and BV CCD observations towards 0311-7651: a region in the Magellanic Bridge where cold atomic Hydrogen has previously been detected by Kobulnicky & Dickey: Additionally, BV images of a comparison held 1 degrees to the South were taken. No CO was detected to a limit of similar to 0.06 Kelvin, and the colour-magnitude diagrams show no evidence for a stellar association in either field.

AB - We present (CO)-C-12(1-0) molecular line and BV CCD observations towards 0311-7651: a region in the Magellanic Bridge where cold atomic Hydrogen has previously been detected by Kobulnicky & Dickey: Additionally, BV images of a comparison held 1 degrees to the South were taken. No CO was detected to a limit of similar to 0.06 Kelvin, and the colour-magnitude diagrams show no evidence for a stellar association in either field.

UR - https://www.scopus.com/pages/publications/0041134580

M3 - Article

SN - 0004-6361

VL - 363

SP - 451

EP - 454

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 2

ER -

CO and optical observations of the Magellanic Bridge

Abstract

ASJC Scopus subject areas

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