ON THE TURNOVER OF THE TULLY-FISHER RELATION

MH RHEE; RF PELETIER; TS VANALBADA

ON THE TURNOVER OF THE TULLY-FISHER RELATION

MH RHEE^*, RF PELETIER, TS VANALBADA

^*Bijbehorende auteur voor dit werk

Rijksuniversiteit Groningen

Onderzoeksoutput › Academic › peer review

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The observed turnover at the high linewidth end of the infrared Tully-Fisher relation can be explained by the stellar population differences among galaxies. When the IRAS 60 mu m fluxes are added to the Tully-Fisher relation as a second parameter, the turnover disappears and the scatter becomes smaller, from 0.35 to 0.25 mag.

Originele taal-2	English
Pagina's (van-tot)	275-277
Aantal pagina's	3
Tijdschrift	Astrophysical letters & communications
Volume	31
Nummer van het tijdschrift	1-6
Status	Published - 1995
Evenement	World of Galaxies II Meeting - , France Duur: 5-sep.-1994 → 7-sep.-1994

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@article{9ea2b05455e94758918e658138d1a120,

title = "ON THE TURNOVER OF THE TULLY-FISHER RELATION",

abstract = "The observed turnover at the high linewidth end of the infrared Tully-Fisher relation can be explained by the stellar population differences among galaxies. When the IRAS 60 mu m fluxes are added to the Tully-Fisher relation as a second parameter, the turnover disappears and the scatter becomes smaller, from 0.35 to 0.25 mag.",

keywords = "GALAXIES, FUNDAMENTAL PARAMETERS, COSMOLOGY, DISTANCE SCALE",

author = "MH RHEE and RF PELETIER and TS VANALBADA",

year = "1995",

language = "English",

volume = "31",

pages = "275--277",

journal = "Astrophysical letters & communications",

issn = "0888-6512",

number = "1-6",

note = "World of Galaxies II Meeting ; Conference date: 05-09-1994 Through 07-09-1994",

}

TY - JOUR

T1 - ON THE TURNOVER OF THE TULLY-FISHER RELATION

AU - RHEE, MH

AU - PELETIER, RF

AU - VANALBADA, TS

PY - 1995

Y1 - 1995

N2 - The observed turnover at the high linewidth end of the infrared Tully-Fisher relation can be explained by the stellar population differences among galaxies. When the IRAS 60 mu m fluxes are added to the Tully-Fisher relation as a second parameter, the turnover disappears and the scatter becomes smaller, from 0.35 to 0.25 mag.

AB - The observed turnover at the high linewidth end of the infrared Tully-Fisher relation can be explained by the stellar population differences among galaxies. When the IRAS 60 mu m fluxes are added to the Tully-Fisher relation as a second parameter, the turnover disappears and the scatter becomes smaller, from 0.35 to 0.25 mag.

KW - GALAXIES, FUNDAMENTAL PARAMETERS

KW - COSMOLOGY, DISTANCE SCALE

M3 - Article

SN - 0888-6512

VL - 31

SP - 275

EP - 277

JO - Astrophysical letters & communications

JF - Astrophysical letters & communications

IS - 1-6

T2 - World of Galaxies II Meeting

Y2 - 5 September 1994 through 7 September 1994

ER -