A search for CO J = 2 → 1 emission from the metal rich globular cluster NGC 6356

M. E. L. Hopwood; S. P S Eyres; A. J. Penny; A. Evans

doi:10.1023/A:1000704132461

A search for CO J = 2 → 1 emission from the metal rich globular cluster NGC 6356

M. E. L. Hopwood, S. P S Eyres, A. J. Penny, A. Evans

Faculty of Computing, Engineering and Science

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

Abstract

We have observed the metal-rich globular cluster NGC 6356 in the CO J = 2 → 1 transition. The data revealed no apparent emission corresponding to the radial velocity of the cluster and we present an upper limit to the mass of gas in the cluster core.

Original language	English
Pages (from-to)	385-388
Number of pages	4
Journal	Astrophysics and Space Science
Volume	251
Issue number	1-2
DOIs	https://doi.org/10.1023/A:1000704132461
Publication status	Published - 1997

Access to Document

10.1023/A:1000704132461

Cite this

@article{4de8cfedbea34a8fa2dfb36ecc6422f5,

title = "A search for CO J = 2 → 1 emission from the metal rich globular cluster NGC 6356",

abstract = "We have observed the metal-rich globular cluster NGC 6356 in the CO J = 2 → 1 transition. The data revealed no apparent emission corresponding to the radial velocity of the cluster and we present an upper limit to the mass of gas in the cluster core.",

author = "Hopwood, {M. E. L.} and Eyres, {S. P S} and Penny, {A. J.} and A. Evans",

year = "1997",

doi = "10.1023/A:1000704132461",

language = "English",

volume = "251",

pages = "385--388",

journal = "Astrophysics and Space Science",

issn = "0004-640X",

publisher = "Springer",

number = "1-2",

}

TY - JOUR

T1 - A search for CO J = 2 → 1 emission from the metal rich globular cluster NGC 6356

AU - Hopwood, M. E. L.

AU - Eyres, S. P S

AU - Penny, A. J.

AU - Evans, A.

PY - 1997

Y1 - 1997

N2 - We have observed the metal-rich globular cluster NGC 6356 in the CO J = 2 → 1 transition. The data revealed no apparent emission corresponding to the radial velocity of the cluster and we present an upper limit to the mass of gas in the cluster core.

AB - We have observed the metal-rich globular cluster NGC 6356 in the CO J = 2 → 1 transition. The data revealed no apparent emission corresponding to the radial velocity of the cluster and we present an upper limit to the mass of gas in the cluster core.

U2 - 10.1023/A:1000704132461

DO - 10.1023/A:1000704132461

M3 - Article

AN - SCOPUS:0040060137

SN - 0004-640X

VL - 251

SP - 385

EP - 388

JO - Astrophysics and Space Science

JF - Astrophysics and Space Science

IS - 1-2

ER -

A search for CO J = 2 → 1 emission from the metal rich globular cluster NGC 6356

Abstract

Access to Document

Fingerprint

Cite this