Millimetre observations of infrared carbon stars - I. The data

M Sevenster; HWW Spoon; I Perez; MAT GROENEWEGEN

doi:10.1051/0004-6361:20020727

Millimetre observations of infrared carbon stars - I. The data

M Sevenster, HWW Spoon, I Perez, MAT GROENEWEGEN^*

^*Corresponding author voor dit werk

Kapteyn Astronomical Institute

Onderzoeksoutput › Academic › peer review

29 Citaten (Scopus)

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Millimetre observations of IRAS selected red carbon stars are presented. About 260 stars have been observed with SEST and IRAM in the CO (1-0) and CO (2-1) lines and partially in HCN (1-0) and SiO (3-2). An overall detection rate, in at least one line, of about 80% is achieved. The survey represents the second largest survey for AGB stars, and the largest ever for carbon stars. Two new detections in SiO (3-2) in carbon stars are reported. When available, the SiO/HCN and HCN/CO (1-0) line ratios are consistent with the ratios expected for carbon stars.

Originele taal-2	English
Pagina's (van-tot)	501-510
Aantal pagina's	10
Tijdschrift	Astronomy & Astrophysics
Volume	390
Nummer van het tijdschrift	2
DOI's	https://doi.org/10.1051/0004-6361:20020727
Status	Published - aug.-2002

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Millimetre observations of infrared carbon stars - I. The data
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Millimetre observations of carbon stars. I.
Groenewegen, M. A. T. (Contributor), Sevenster, M. (Contributor), Spoon, H. (Contributor) & Pérez, I. (Contributor), Strasbourg Astronomical Data Center, 16-jul.-2002
DOI: 10.26093/cds/vizier.33900501
Dataset
Millimetre observations of carbon stars. II.
Groenewegen, M. A. T. (Contributor), Sevenster, M. (Contributor), Spoon, H. (Contributor) & Pérez, I. (Contributor), Strasbourg Astronomical Data Center, 16-jul.-2002
DOI: 10.26093/cds/vizier.33900511, https://doi.org/10.26093%2Fcds%2Fvizier.33900511
Dataset

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title = "Millimetre observations of infrared carbon stars - I. The data",

abstract = "Millimetre observations of IRAS selected red carbon stars are presented. About 260 stars have been observed with SEST and IRAM in the CO (1-0) and CO (2-1) lines and partially in HCN (1-0) and SiO (3-2). An overall detection rate, in at least one line, of about 80% is achieved. The survey represents the second largest survey for AGB stars, and the largest ever for carbon stars. Two new detections in SiO (3-2) in carbon stars are reported. When available, the SiO/HCN and HCN/CO (1-0) line ratios are consistent with the ratios expected for carbon stars.",

keywords = "circumstellar matter, stars : mass-loss, stars : AGB and post-AGB, CIRCUMSTELLAR ENVELOPES, RADIAL-VELOCITIES, HCN OBSERVATIONS, JHK PHOTOMETRY, GALACTIC PLANE, EVOLVED STARS, IRAS SOURCES, AGB STARS, CO, CANDIDATES",

author = "M Sevenster and HWW Spoon and I Perez and MAT GROENEWEGEN",

year = "2002",

month = aug,

doi = "10.1051/0004-6361:20020727",

language = "English",

volume = "390",

pages = "501--510",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

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TY - JOUR

T1 - Millimetre observations of infrared carbon stars - I. The data

AU - Sevenster, M

AU - Spoon, HWW

AU - Perez, I

AU - GROENEWEGEN, MAT

PY - 2002/8

Y1 - 2002/8

N2 - Millimetre observations of IRAS selected red carbon stars are presented. About 260 stars have been observed with SEST and IRAM in the CO (1-0) and CO (2-1) lines and partially in HCN (1-0) and SiO (3-2). An overall detection rate, in at least one line, of about 80% is achieved. The survey represents the second largest survey for AGB stars, and the largest ever for carbon stars. Two new detections in SiO (3-2) in carbon stars are reported. When available, the SiO/HCN and HCN/CO (1-0) line ratios are consistent with the ratios expected for carbon stars.

AB - Millimetre observations of IRAS selected red carbon stars are presented. About 260 stars have been observed with SEST and IRAM in the CO (1-0) and CO (2-1) lines and partially in HCN (1-0) and SiO (3-2). An overall detection rate, in at least one line, of about 80% is achieved. The survey represents the second largest survey for AGB stars, and the largest ever for carbon stars. Two new detections in SiO (3-2) in carbon stars are reported. When available, the SiO/HCN and HCN/CO (1-0) line ratios are consistent with the ratios expected for carbon stars.

KW - circumstellar matter

KW - stars : mass-loss

KW - stars : AGB and post-AGB

KW - CIRCUMSTELLAR ENVELOPES

KW - RADIAL-VELOCITIES

KW - HCN OBSERVATIONS

KW - JHK PHOTOMETRY

KW - GALACTIC PLANE

KW - EVOLVED STARS

KW - IRAS SOURCES

KW - AGB STARS

KW - CO

KW - CANDIDATES

U2 - 10.1051/0004-6361:20020727

DO - 10.1051/0004-6361:20020727

M3 - Article

SN - 0004-6361

VL - 390

SP - 501

EP - 510

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

IS - 2

ER -

Millimetre observations of infrared carbon stars - I. The data

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Millimetre observations of carbon stars. I.

Millimetre observations of carbon stars. II.

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